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1994-06-04
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41KB
Date: Fri, 3 Dec 93 06:03:33 PST
From: Info-Hams Mailing List and Newsgroup <info-hams@ucsd.edu>
Errors-To: Info-Hams-Errors@UCSD.Edu
Reply-To: Info-Hams@UCSD.Edu
Precedence: Bulk
Subject: Info-Hams Digest V93 #1419
To: Info-Hams
Info-Hams Digest Fri, 3 Dec 93 Volume 93 : Issue 1419
Today's Topics:
Alinco DJF1T-HP dead
ARLD065 DX news
Daily Summary of Solar Geophysical Activity for 27 November
Daily Summary of Solar Geophysical Activity for 28 November
Daily Summary of Solar Geophysical Activity for 29 November
Penn State ARC still exists!
Pyramid Schemes
The Power of Photons
Send Replies or notes for publication to: <Info-Hams@UCSD.Edu>
Send subscription requests to: <Info-Hams-REQUEST@UCSD.Edu>
Problems you can't solve otherwise to brian@ucsd.edu.
Archives of past issues of the Info-Hams Digest are available
(by FTP only) from UCSD.Edu in directory "mailarchives/info-hams".
We trust that readers are intelligent enough to realize that all text
herein consists of personal comments and does not represent the official
policies or positions of any party. Your mileage may vary. So there.
----------------------------------------------------------------------
Date: 3 Dec 93 13:35:00 GMT
From: news-mail-gateway@ucsd.edu
Subject: Alinco DJF1T-HP dead
To: info-hams@ucsd.edu
> I purchased a new ALINCO DJF1T-HP, and ever since the day I bought it, I
> have been having problems with it. The first problem was with the
> keyboard lighting (only half of the keyboard would light). Then I have
> been having problems with the internal ribbon cables, which would
> intermittently cause loss of certain functions. And just recently,
> the radio started to smoke and has ceased to function at all (now
> at the shop for gut replacement) :(.
> Has anyone had any problems with their ALINCO DJF1T-HP?
>
> Thanks.
>
I have a DJF1T and it has performed perfectly!. I've had it for
just over a year.
Hope it gets fixed to your satifaction.
73
TJ kv2x
--
-------------------------------------------------------------
|
Thomas J. Jennings | Tel: (716) 273 7071
Development Engineer | Fax: (716) 273 7262
|
ABB Process Automation |
Post Office Box 22685 |
Rochester, New York 14692-2685 |
|
-------------------------------------------------------------
Internet: jennings@jennings.rochny.uspra.abb.com
-------------------------------------------------------------
------------------------------
Date: Wed, 1 Dec 1993 05:36:56 -0700
From: tribune.usask.ca!kakwa.ucs.ualberta.ca!alberta!nebulus!ve6mgs!usenet@decwrl.dec.com
Subject: ARLD065 DX news
To: info-hams@ucsd.edu
SB DX @ ARL $ARLD065
ARLD065 DX news
ZCZC AE91
QST de W1AW
DX Bulletin 65 ARLD065
------------------------------
Date: Sat, 27 Nov 1993 21:01:28 MST
From: tribune.usask.ca!kakwa.ucs.ualberta.ca!alberta!nebulus!ve6mgs!usenet@decwrl.dec.com
Subject: Daily Summary of Solar Geophysical Activity for 27 November
To: info-hams@ucsd.edu
/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\
DAILY SUMMARY OF SOLAR GEOPHYSICAL ACTIVITY
27 NOVEMBER, 1993
/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\
(Based In-Part On SESC Observational Data)
SOLAR AND GEOPHYSICAL ACTIVITY INDICES FOR 27 NOVEMBER, 1993
------------------------------------------------------------
!!BEGIN!! (1.0) S.T.D. Solar Geophysical Data Broadcast for DAY 331, 11/27/93
10.7 FLUX=090 90-AVG=094 SSN=055 BKI=2100 0112 BAI=002
BGND-XRAY=A8.5 FLU1=4.2E+05 FLU10=1.3E+04 PKI=2100 1212 PAI=004
BOU-DEV=017,008,003,003,004,007,007,016 DEV-AVG=008 NT SWF=00:000
XRAY-MAX= B3.2 @ 2049UT XRAY-MIN= A7.8 @ 1813UT XRAY-AVG= B1.1
NEUTN-MAX= +001% @ 2305UT NEUTN-MIN= -002% @ 1025UT NEUTN-AVG= -0.1%
PCA-MAX= +0.3DB @ 1400UT PCA-MIN= -0.5DB @ 1310UT PCA-AVG= +0.1DB
BOUTF-MAX=55364NT @ 0316UT BOUTF-MIN=55345NT @ 1931UT BOUTF-AVG=55357NT
GOES7-MAX=P:+000NT@ 0000UT GOES7-MIN=N:+000NT@ 0000UT G7-AVG=+063,+000,+000
GOES6-MAX=P:+116NT@ 2002UT GOES6-MIN=N:-058NT@ 1117UT G6-AVG=+085,+017,-032
FLUXFCST=STD:090,090,090;SESC:090,090,090 BAI/PAI-FCST=005,005,018/010,010,030
KFCST=2223 3222 2223 3222 27DAY-AP=007,008 27DAY-KP=1132 2223 2222 3232
WARNINGS=*SWF
ALERTS=
!!END-DATA!!
NOTE: The Effective Sunspot Number for 26 NOV 93 was 44.0.
The Full Kp Indices for 26 NOV 93 are: 2o 2- 1+ 2- 2o 3- 4o 2+
SYNOPSIS OF ACTIVITY
--------------------
Solar activity was very low. Several B-class x-ray bursts
occurred, none of which were optically correlated. All sunspot
regions appeared to be stable.
Solar activity forecast: solar activity is expected to be
very low to low. Region 7620 (N04W53) could produce an isolated
C-class subflare.
The geomagnetic field has been at mostly quiet levels for the
past 24 hours.
Geophysical activity forecast: the geomagnetic field is
expected to be at quiet to unsettled levels during the first
two days. Activity will increase to active to minor storm
levels on the final day due to coronal hole effects.
Event probabilities 28 nov-30 nov
Class M 01/01/01
Class X 01/01/01
Proton 01/01/01
PCAF Green
Geomagnetic activity probabilities 28 nov-30 nov
A. Middle Latitudes
Active 10/10/20
Minor Storm 05/05/20
Major-Severe Storm 01/01/15
B. High Latitudes
Active 10/10/20
Minor Storm 05/05/25
Major-Severe Storm 01/01/20
HF propagation conditions were normal over all regions.
Similar conditions will persist through 29 November inclusive.
Minor signal degradation is expected on 30 November for
transpolar and transauroral paths as a recurrent coronal-hole-
related disturbance begins to arrive. Stronger and more
widespread ionospheric activity is expected to take effect on
01 and/or 02 December.
COPIES OF JOINT USAF/NOAA SESC SOLAR GEOPHYSICAL REPORTS
========================================================
REGIONS WITH SUNSPOTS. LOCATIONS VALID AT 27/2400Z NOVEMBER
-----------------------------------------------------------
NMBR LOCATION LO AREA Z LL NN MAG TYPE
7620 N03W53 268 0190 EAO 12 017 BETA
7622 N12W07 222 0010 BXO 03 005 BETA
7623 S12E54 161 0030 CSO 06 003 BETA
7621 S09W43 258 PLAGE
REGIONS DUE TO RETURN 28 NOVEMBER TO 30 NOVEMBER
NMBR LAT LO
NONE
LISTING OF SOLAR ENERGETIC EVENTS FOR 27 NOVEMBER, 1993
-------------------------------------------------------
BEGIN MAX END RGN LOC XRAY OP 245MHZ 10CM SWEEP
NONE
POSSIBLE CORONAL MASS EJECTION EVENTS FOR 27 NOVEMBER, 1993
-----------------------------------------------------------
BEGIN MAX END LOCATION TYPE SIZE DUR II IV
NO EVENTS OBSERVED
INFERRED CORONAL HOLES. LOCATIONS VALID AT 27/2400Z
---------------------------------------------------
ISOLATED HOLES AND POLAR EXTENSIONS
EAST SOUTH WEST NORTH CAR TYPE POL AREA OBSN
51 N70E87 S10E47 N15E01 N70E87 190 EXT POS 049 10830A
52 S05E02 S12W02 S12W15 S01W02 226 ISO NEG 004 10830A
SUMMARY OF FLARE EVENTS FOR THE PREVIOUS UTC DAY
------------------------------------------------
Date Begin Max End Xray Op Region Locn 2695 MHz 8800 MHz 15.4 GHz
------ ---- ---- ---- ---- -- ------ ------ --------- --------- ---------
26 Nov: 0049 0104 0125 B3.7
0159 0203 0205 B3.8
0720 0725 0729 B4.0 SF 7622 N12E17
1117 1130 1142 B3.8
1150 1211 1212 B4.3
1320 1325 1328 B5.6
1558 1605 1608 C2.1 SF 7623 S09E75
1702 1712 1721 C1.2 SF 7620 N04W38
1958 2003 2007 B4.2 SF 7620 N02W43
REGION FLARE STATISTICS FOR THE PREVIOUS UTC DAY
------------------------------------------------
C M X S 1 2 3 4 Total (%)
-- -- -- -- -- -- -- -- --- ------
Region 7620: 1 0 0 2 0 0 0 0 002 (22.2)
Region 7622: 0 0 0 1 0 0 0 0 001 (11.1)
Region 7623: 1 0 0 1 0 0 0 0 001 (11.1)
Uncorrellated: 0 0 0 0 0 0 0 0 005 (55.6)
Total Events: 009 optical and x-ray.
EVENTS WITH SWEEPS AND/OR OPTICAL PHENOMENA FOR THE LAST UTC DAY
----------------------------------------------------------------
Date Begin Max End Xray Op Region Locn Sweeps/Optical Observations
------ ---- ---- ---- ---- -- ------ ------ ---------------------------
NO EVENTS OBSERVED.
NOTES:
All times are in Universal Time (UT). Characters preceding begin, max,
and end times are defined as: B = Before, U = Uncertain, A = After.
All times associated with x-ray flares (ex. flares which produce
associated x-ray bursts) refer to the begin, max, and end times of the
x-rays. Flares which are not associated with x-ray signatures use the
optical observations to determine the begin, max, and end times.
Acronyms used to identify sweeps and optical phenomena include:
II = Type II Sweep Frequency Event
III = Type III Sweep
IV = Type IV Sweep
V = Type V Sweep
Continuum = Continuum Radio Event
Loop = Loop Prominence System,
Spray = Limb Spray,
Surge = Bright Limb Surge,
EPL = Eruptive Prominence on the Limb.
** End of Daily Report **
------------------------------
Date: Mon, 29 Nov 1993 00:38:40 MST
From: tribune.usask.ca!kakwa.ucs.ualberta.ca!alberta!ugc!nebulus!ve6mgs!usenet@decwrl.dec.com
Subject: Daily Summary of Solar Geophysical Activity for 28 November
To: info-hams@ucsd.edu
/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\
DAILY SUMMARY OF SOLAR GEOPHYSICAL ACTIVITY
28 NOVEMBER, 1993
/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\
(Based In-Part On SESC Observational Data)
SOLAR AND GEOPHYSICAL ACTIVITY INDICES FOR 28 NOVEMBER, 1993
------------------------------------------------------------
!!BEGIN!! (1.0) S.T.D. Solar Geophysical Data Broadcast for DAY 332, 11/28/93
10.7 FLUX=093 90-AVG=094 SSN=075 BKI=0001 2111 BAI=002
BGND-XRAY=B1.4 FLU1=6.0E+05 FLU10=1.2E+04 PKI=1101 2211 PAI=004
BOU-DEV=004,004,004,009,012,008,006,006 DEV-AVG=006 NT SWF=00:000
XRAY-MAX= B7.4 @ 0103UT XRAY-MIN= B1.1 @ 0501UT XRAY-AVG= B1.9
NEUTN-MAX= +002% @ 1945UT NEUTN-MIN= -002% @ 0835UT NEUTN-AVG= +0.3%
PCA-MAX= +0.1DB @ 1125UT PCA-MIN= -0.5DB @ 1340UT PCA-AVG= +0.0DB
BOUTF-MAX=55363NT @ 0047UT BOUTF-MIN=55338NT @ 1911UT BOUTF-AVG=55354NT
GOES7-MAX=P:+000NT@ 0000UT GOES7-MIN=N:+000NT@ 0000UT G7-AVG=+073,+000,+000
GOES6-MAX=P:+117NT@ 1754UT GOES6-MIN=N:-058NT@ 1036UT G6-AVG=+095,+017,-031
FLUXFCST=STD:095,095,095;SESC:095,095,095 BAI/PAI-FCST=010,018,051/010,025,070
KFCST=1112 3334 3344 3334 27DAY-AP=008,004 27DAY-KP=2222 3232 2121 1211
WARNINGS=*SWF;*MAJSTRM;*AURMIDWRN
ALERTS=
!!END-DATA!!
NOTE: The Effective Sunspot Number for 27 NOV 93 was 42.0.
The Full Kp Indices for 27 NOV 93 are: 2o 1+ 0+ 0o 1+ 2- 1+ 2o
SYNOPSIS OF ACTIVITY
--------------------
Solar activity was very low. A single B-class subflare
occurred. New Regions 7624 (N03E13) and 7625 (S14E14) were
numbered. Region 7625 showed gradual growth during the day.
Solar activity forecast: solar activity is expected to be
very low to low. Region 7625 could produce an isolated C-class
subflare.
The geomagnetic field has been at mostly quiet levels for the
past 24 hours.
Geophysical activity forecast: the geomagnetic field is
expected to be at mostly unsettled levels during the first
day. Coronal hole effects are expected to increase activity to
active levels during the second day, then major storm levels
on the final day. Brief periods of severe storming could occur
late in the period as well.
Event probabilities 29 nov-01 dec
Class M 10/10/10
Class X 01/01/01
Proton 01/01/01
PCAF Green
Geomagnetic activity probabilities 29 nov-01 dec
A. Middle Latitudes
Active 35/35/20
Minor Storm 15/15/25
Major-Severe Storm 10/10/40
B. High Latitudes
Active 35/35/20
Minor Storm 20/20/20
Major-Severe Storm 10/10/50
HF propagation conditions continued normal over all
regions. Conditions will continue near-normal on 29 November
and should remain near-normal for a fair portion of 30
November, although signal degradation over the high and polar
latitude paths will begin to affect communications on these
higher latitude paths. Very poor to occasionally useless
propagation is expected on 01 and 02 December (with emphasis on
01 December) in response to the anticipated major geomagnetic
storm. Middle latitudes are expected to see fair to
occasionally very poor propagation with strongest signal
degradation occuring during the local night and sunrise
sectors. If recurrence is any indication, full recovery from
this disturbance will not likely be observed for at least 2 to
4 days after the geomagnetic storming ends (on 02 or
03 December).
COPIES OF JOINT USAF/NOAA SESC SOLAR GEOPHYSICAL REPORTS
========================================================
REGIONS WITH SUNSPOTS. LOCATIONS VALID AT 28/2400Z NOVEMBER
-----------------------------------------------------------
NMBR LOCATION LO AREA Z LL NN MAG TYPE
7620 N03W68 270 0210 CAO 09 008 BETA
7622 N13W20 222 0010 AXX 03 004 ALPHA
7623 S10E41 161 0020 CRO 01 002 BETA
7624 N03E13 189 0020 BXO 03 005 BETA
7625 S14E14 188 0020 CRO 03 006 BETA
7621 S09W56 258 PLAGE
REGIONS DUE TO RETURN 29 NOVEMBER TO 01 DECEMBER
NMBR LAT LO
NONE
LISTING OF SOLAR ENERGETIC EVENTS FOR 28 NOVEMBER, 1993
-------------------------------------------------------
BEGIN MAX END RGN LOC XRAY OP 245MHZ 10CM SWEEP
NONE
POSSIBLE CORONAL MASS EJECTION EVENTS FOR 28 NOVEMBER, 1993
-----------------------------------------------------------
BEGIN MAX END LOCATION TYPE SIZE DUR II IV
NO EVENTS OBSERVED
INFERRED CORONAL HOLES. LOCATIONS VALID AT 28/2400Z
---------------------------------------------------
ISOLATED HOLES AND POLAR EXTENSIONS
EAST SOUTH WEST NORTH CAR TYPE POL AREA OBSN
NO DATA AVAILABLE FOR ANALYSIS
SUMMARY OF FLARE EVENTS FOR THE PREVIOUS UTC DAY
------------------------------------------------
Date Begin Max End Xray Op Region Locn 2695 MHz 8800 MHz 15.4 GHz
------ ---- ---- ---- ---- -- ------ ------ --------- --------- ---------
27 Nov: 0109 0117 0126 B2.5
0219 0223 0229 B2.2
0336 0339 0343 B1.7
0348 0412 0438 B3.0
0546 0552 0559 B2.1
1251 1254 1258 B1.5
2042 2049 2054 B3.2
REGION FLARE STATISTICS FOR THE PREVIOUS UTC DAY
------------------------------------------------
C M X S 1 2 3 4 Total (%)
-- -- -- -- -- -- -- -- --- ------
Uncorrellated: 0 0 0 0 0 0 0 0 007 (100.0)
Total Events: 007 optical and x-ray.
EVENTS WITH SWEEPS AND/OR OPTICAL PHENOMENA FOR THE LAST UTC DAY
----------------------------------------------------------------
Date Begin Max End Xray Op Region Locn Sweeps/Optical Observations
------ ---- ---- ---- ---- -- ------ ------ ---------------------------
NO EVENTS OBSERVED.
NOTES:
All times are in Universal Time (UT). Characters preceding begin, max,
and end times are defined as: B = Before, U = Uncertain, A = After.
All times associated with x-ray flares (ex. flares which produce
associated x-ray bursts) refer to the begin, max, and end times of the
x-rays. Flares which are not associated with x-ray signatures use the
optical observations to determine the begin, max, and end times.
Acronyms used to identify sweeps and optical phenomena include:
II = Type II Sweep Frequency Event
III = Type III Sweep
IV = Type IV Sweep
V = Type V Sweep
Continuum = Continuum Radio Event
Loop = Loop Prominence System,
Spray = Limb Spray,
Surge = Bright Limb Surge,
EPL = Eruptive Prominence on the Limb.
** End of Daily Report **
------------------------------
Date: Mon, 29 Nov 1993 23:10:31 MST
From: tribune.usask.ca!kakwa.ucs.ualberta.ca!alberta!nebulus!ve6mgs!usenet@decwrl.dec.com
Subject: Daily Summary of Solar Geophysical Activity for 29 November
To: info-hams@ucsd.edu
/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\
DAILY SUMMARY OF SOLAR GEOPHYSICAL ACTIVITY
29 NOVEMBER, 1993
/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\
(Based In-Part On SESC Observational Data)
SOLAR AND GEOPHYSICAL ACTIVITY INDICES FOR 29 NOVEMBER, 1993
------------------------------------------------------------
!!BEGIN!! (1.0) S.T.D. Solar Geophysical Data Broadcast for DAY 333, 11/29/93
10.7 FLUX=093.8 90-AVG=094 SSN=092 BKI=4212 2221 BAI=008
BGND-XRAY=B1.9 FLU1=6.6E+05 FLU10=1.2E+04 PKI=4222 2222 PAI=008
BOU-DEV=040,010,008,011,010,010,010,008 DEV-AVG=013 NT SWF=00:000
XRAY-MAX= C2.1 @ 2317UT XRAY-MIN= B1.5 @ 0136UT XRAY-AVG= B2.7
NEUTN-MAX= +003% @ 0550UT NEUTN-MIN= -001% @ 2300UT NEUTN-AVG= +0.4%
PCA-MAX= +0.0DB @ 2355UT PCA-MIN= -0.5DB @ 1410UT PCA-AVG= -0.1DB
BOUTF-MAX=55360NT @ 0221UT BOUTF-MIN=55335NT @ 1915UT BOUTF-AVG=55351NT
GOES7-MAX=P:+000NT@ 0000UT GOES7-MIN=N:+000NT@ 0000UT G7-AVG=+063,+000,+000
GOES6-MAX=P:+123NT@ 1714UT GOES6-MIN=N:-055NT@ 1028UT G6-AVG=+086,+017,-029
FLUXFCST=STD:095,095,095;SESC:095,095,095 BAI/PAI-FCST=018,051,025/025,070,030
KFCST=3344 3334 5566 6655 27DAY-AP=004,008 27DAY-KP=2121 1211 1011 2234
WARNINGS=*SWF;*MAJSTRM;*AURMIDWRN
ALERTS=
!!END-DATA!!
NOTE: The Effective Sunspot Number for 28 NOV 93 was 42.3.
The Full Kp Indices for 28 NOV 93 are: 1- 1o 0+ 1o 2o 2- 1o 1+
SYNOPSIS OF ACTIVITY
--------------------
Solar activity was low. Three C-class x-ray bursts
occurred and were probably produced by new Region 7627
(S19E85). Active surge and prominence activity accompanied the
region as it rotated into view midway through the period. New
Region 7626 (N28E12) was also numbered.
STD: Strong Ca XV emissions were observed today on the
southeast limb centered at S19, spanning from S31 to S10.
These emissions were also accompanied by strong Fe X and Fe XIV
emissions. Weak Ca XV emissions were observed yesterday.
This area is also bright in x-rays, as seen by the Yohkoh
satellite. A full-disk Yohkoh image has been reduced and
appended to this report. The large northern polar coronal hole
extension is also clearly visible, approaching the central
meridian at 00:40 UTC on 29 November.
Solar activity forecast: solar activity is expected to be
low. Region 7627 may continue to produce C-class activity.
The geomagnetic field has been at quiet to unsettled levels
for the past 24 hours. Isolated active periods also occurred.
Geophysical activity forecast: the geomagnetic field is
expected to be at unsettled to active levels during the first
day increasing to major storm levels during the second day.
Brief severe storm periods could also occur during the second
day, particularly at high latitudes. Activity is expected to
decline to active to minor storm levels during the final day.
This activity is expected due to recurrent coronal hole
effects.
Event probabilities 30 nov-02 dec
Class M 10/10/10
Class X 01/01/01
Proton 01/01/01
PCAF Green
Geomagnetic activity probabilities 30 nov-02 dec
A. Middle Latitudes
Active 35/20/35
Minor Storm 15/25/25
Major-Severe Storm 10/40/20
B. High Latitudes
Active 35/20/30
Minor Storm 20/20/30
Major-Severe Storm 10/50/20
HF propagation conditions were normal over all regions.
Tommorrow (30 November) should see the last period of stable
ionospheric communications. Late on 30 November and/or
particularly on 01 December, conditions are expected to become
substantially disturbed. High and polar latitude paths are
expected to become frequently useless, particularly during
the local night and sunrise sectors due to potentially strong
geomagnetic and auroral storm activity. These effects should
also migrate to the middle-latitude regions, affecting many
middle-latitude paths and limiting propagation to more
north-south oriented paths. Conditions are not expected
improve for several days after the storming subsides, but
should have returned to near-normal by about 04 or 05 December.
NOTE that there is a chance for VHF auroral backscatter during
the most disturbed periods (geomagnetic K-indices of 6 or
more). Please report VHF and or other unusual or interesting
HF/VHF contacts during this period to: COler@Solar.Stanford.Edu.
COPIES OF JOINT USAF/NOAA SESC SOLAR GEOPHYSICAL REPORTS
========================================================
REGIONS WITH SUNSPOTS. LOCATIONS VALID AT 29/2400Z NOVEMBER
-----------------------------------------------------------
NMBR LOCATION LO AREA Z LL NN MAG TYPE
7620 N04W85 273 0150 HSX 02 001 ALPHA
7623 S11E27 161 0020 HRX 01 001 ALPHA
7624 N03W00 188 0030 CRO 06 009 BETA
7625 S15E01 187 0050 DSO 06 016 BETA
7626 N28E12 176 0010 BXO 04 004 BETA
7627 S19E85 103 0050 HSX 01 001 ALPHA
7622 N14W34 222 PLAGE
REGIONS DUE TO RETURN 30 NOVEMBER TO 02 DECEMBER
NMBR LAT LO
NONE
LISTING OF SOLAR ENERGETIC EVENTS FOR 29 NOVEMBER, 1993
-------------------------------------------------------
A. ENERGETIC EVENTS:
BEGIN MAX END RGN LOC XRAY OP 245MHZ 10CM SWEEP
2027 2028 2028 110
POSSIBLE CORONAL MASS EJECTION EVENTS FOR 29 NOVEMBER, 1993
-----------------------------------------------------------
BEGIN MAX END LOCATION TYPE SIZE DUR II IV
29/ 2158 A2344 S29E90 EPL C2.1 27
INFERRED CORONAL HOLES. LOCATIONS VALID AT 29/2400Z
---------------------------------------------------
ISOLATED HOLES AND POLAR EXTENSIONS
EAST SOUTH WEST NORTH CAR TYPE POL AREA OBSN
51 N57E87 S11W06 N25W24 N60W01 180 EXT POS 095 10830A
SUMMARY OF FLARE EVENTS FOR THE PREVIOUS UTC DAY
------------------------------------------------
Date Begin Max End Xray Op Region Locn 2695 MHz 8800 MHz 15.4 GHz
------ ---- ---- ---- ---- -- ------ ------ --------- --------- ---------
28 Nov: 0050 0102 0109 B7.4 SF 7623 S11E49
REGION FLARE STATISTICS FOR THE PREVIOUS UTC DAY
------------------------------------------------
C M X S 1 2 3 4 Total (%)
-- -- -- -- -- -- -- -- --- ------
Region 7623: 0 0 0 1 0 0 0 0 001 (100.0)
Uncorrellated: 0 0 0 0 0 0 0 0 000 ( 0.0)
Total Events: 001 optical and x-ray.
EVENTS WITH SWEEPS AND/OR OPTICAL PHENOMENA FOR THE LAST UTC DAY
----------------------------------------------------------------
Date Begin Max End Xray Op Region Locn Sweeps/Optical Observations
------ ---- ---- ---- ---- -- ------ ------ ---------------------------
NO EVENTS OBSERVED.
NOTES:
All times are in Universal Time (UT). Characters preceding begin, max,
and end times are defined as: B = Before, U = Uncertain, A = After.
All times associated with x-ray flares (ex. flares which produce
associated x-ray bursts) refer to the begin, max, and end times of the
x-rays. Flares which are not associated with x-ray signatures use the
optical observations to determine the begin, max, and end times.
Acronyms used to identify sweeps and optical phenomena include:
II = Type II Sweep Frequency Event
III = Type III Sweep
IV = Type IV Sweep
V = Type V Sweep
Continuum = Continuum Radio Event
Loop = Loop Prominence System,
Spray = Limb Spray,
Surge = Bright Limb Surge,
EPL = Eruptive Prominence on the Limb.
SPECIAL INSERT: CURRENT X-RAY EMISSIONS FROM THE JAPANESE YOHKOH SPACECRAFT
===========================================================================
29 November 1993, 00:40 UTC
North
... .. ... ........,,,:::,,,,,,....
.......... ..,,,:,,,,::;;;;;::::,,,,,....
.. .....,,,,.. ...,,:::,,,:::::,,::;;;::::::,,,....
.......,,,,,::,. .,,,,....,,,,,,,,,,,,,::;;;;;:::,,,...
...,,,,,:::::,.. ....... .........,,,,,,,,,,,:,::::;;;;;;::,,... .
....,,,,::::;:,... ..,,.,,,,,,. .,.,,,,,,,,,,::::::::;::;+--;:::,,.....
...,,,:::;;;:;:,,,..,;;;:,::::,... . ..,,,::::::;::::::;::::;;;-;;;:::,,,..
...,:::;;;;:::,::,..;|!!|;::::,,,. .,,::;;;;;;;;;:;;;;;;;;;;;;;;;::::,,,
..,,,::;;---;::::::,,,--!!!+;:::... . ..,,;;---------;;;;;;;;;;;;;;;;;:::,
.,,:::;;-;;;;::::;;;::,.,--;,,... ...:;;-+||||||+------;;;;;;---;;;::
.,,::;;-;;;;;::,,::::,,. . .. ....,,:;-+|!!!||||+----------++--;;;;
,:::;;;;:::::::::::::::.. . ... .,::::;+**111!!||||+--++++++++++---;;
,::;;--;:;;;;;::;;:::,,,....,,..... .,:;:;:;-11|+||++++|---+!!!|!11|+++-;;
::;;---;::;;;;;;-;;;;:,,,. ..,:|+::,... .,:::;;;--++---++---;-++|!!12##3!!+-;:
:;;--+-;;;-----+--;-;;:,.. ..,;22+;:... ..,,::::;;;-------;;;;;--+||!1**41+-;;:
:;;--++---++|!|!!|-;::;:.....,,,,,,, ..,,,,:::::::;;;;;;::::;;;----|34!|-;;:,
:;--+|2!+++|!12221|-;,,..,.,,,:,,.......,,:::,::::::::::::::::::;;;;--+||+;::,,
:;--+!33|++!123421!+;;,,:;;;;-+-;:,....,,,:::::::::::::::::::::::;;-;;;;+-;:,,,
:-+|14#@3|!!12221!2|+--------|1**!:,,,,,,,,:,:::::::::::;::,,::::;;-;:::-;::,,.
:;+|14#@@1|||1221!|+;----;;-+!222|:,,:::,::,,::::,,,,,,:,,,,,,,,,:;::,:;;;:,,,,
:;;-|13##3++-+|||||-;;;;-++|!!!+::::::::::,:,,,,,,.,,.,,,,,,,,,,::,,,:;;;:,,,..
::;-|12321|-------;::::;;;----;::::;;;:;::,,,,,,,,,.,...,,,,,,,::::::;;;:,,....
,:;-|!!!||||-;;;;;:;;;;;;;;::::;;;;;:::::::,,,,,,.,....,....,,,,,::;;;;::,,....
.,::;----++++-;:;;;:::::::::::::::::::,,,,,,,,,.,..,,,,,,,,,,,,:::;;;:::,.... .
..,,::;;;;;;---;;::::::::::::::,,,,,,,,,,,,,,,,.,..,,,,,,,,,,:::;;;:::,,,.
...,,:::;;;;;;;;-;;::::::,,,,,,,,,,,,,,,,,,,,,,,,,,,,,,,,,,:::;;:::,,.....
...,,,:::::;;;;;----;::::::::,,,,,,,...,,...,,,... ...,.,,,,,,,,....
....,,,,,:::;;;;-------;;::::::,,,,....
.......,,,,:::;;;;;;;;;::,,,,,,,,.... .
......,,,,,,,::::,,,..............
... ............ . . .
.
South
KEY: East and west limbs are to the left and right respectively. Emission
strength, from minimum to maximum are coded in the following way:
[space] . , : ; - + | ! 1 2 3 4 * # @
Units used are arbitrary, for illustrative purposes. Get "showasc.zip"
from "pub/solar/Software" at the anonymous FTP site: xi.uleth.ca
(IP # 142.66.3.29) to view these images on VGA screens.
** End of Daily Report **
------------------------------
Date: Wed, 1 Dec 1993 22:56:53 EST
From: ucsnews!sol.ctr.columbia.edu!spool.mu.edu!uwm.edu!psuvax1!psuvm!dcr117@network.ucsd.edu
Subject: Penn State ARC still exists!
To: info-hams@ucsd.edu
Hello netters,
(Particularly Penn State Students, Faculty, Staff, and Alumni)
This is a brief note telling all of you that the Penn State ARC is still
alive. As the Vice-President, I am interested in hearing from some of you
who are or were in the Penn State system. If you are a current student,
or faculty/staff member, you can be a part of the Penn State ARC (PSARC).
Contact me at my E-Mail address for info. (dcr117@psuvm.psu.edu) or via
packet radio (n2oqn@w3ya.pa.usa.noam)
If you are an one of PSU's vast alumni, let me know how you are doing/what
you are up to. We would all be interested in hearing from you guys, and
sharing interesting college stories/ham radio stories at our meetings.
To let you know where the club is/has been going I'll tell you a little bit
about the station...
We are running the following equipment:
Kenwood TS940S HF Rig
Kenwood TS820S HF Rig
Dentron MLA-2500B Linear
Heathkit SB-220 Linear
Mosley TH7DX 7 Element Tribander
Yaesu FT736R 2/440 Satellite Rig
AEA PK-232MBX for RTTY, Packet, etc...
(And other assorted stuff...)
Projects in the works are, completion of a 2/440 Satellite antenna array,
replacement of a terminal for packet/data operation, antenna and
tower maintainence, and other stuff... (I have probably forgotten many
things...)
So, let me know what you guys are doing... Again, reply to this message,
or send packet mail to n2oqn@w3ya.pa.usa.noam.
Thanks and 73,
Dan Raneri (N2OQN)
Vice President,
Penn State Amateur Radio Club
------------------------------
Date: Wed, 1 Dec 1993 09:54:04 GMT
From: cs.utexas.edu!utnut!torn!nott!cunews!freenet.carleton.ca!Freenet.carleton.ca!aj467@uunet.uu.net
Subject: Pyramid Schemes
To: info-hams@ucsd.edu
When you see this crap on the net, everyone of you should reply E-mail to
the originators account, with the entire message intact. Maybe his local
node will boot him off the air. Maybe they'll catch wind and turn him in.
What do you think.
--
Bill VE3NJW Advanced Amateur
Packet Address : VE3NJW@VE3KYT.#EON.ON.CAN
Freenet Address: aj467@Freenet.Carleton.ca
------------------------------
Date: Wed, 1 Dec 1993 09:36:34 GMT
From: europa.eng.gtefsd.com!howland.reston.ans.net!cs.utexas.edu!utnut!torn!nott!cunews!freenet.carleton.ca!Freenet.carleton.ca!aj467@uunet.uu.net
Subject: The Power of Photons
To: info-hams@ucsd.edu
In a previous article, dstock@hpqmoca.sqf.hp.com (David Stockton) says:
> Did he then go on to explain how a photon torpedo worked ?
>
> Cheers,
> David GM4ZNX
>
No I did not explain photon torpedoes. However I made one tonight with an
HF amplifier accident. Fortunately for me I'm still here to read this
message. We still have headaches from the 40 amp 110 volt component that
flew out of the case in great fury, trying to catch the RF that was
generated for the split second of plasma flash. I'm not throwing that
switch tomorrow night ... someone else can do that.
Now as to the Photon energy thing, I have only one question.
What type of wine, a red or a white, is best served with crow.
Can you recommend a good Label or vintage.
--
Bill VE3NJW Advanced Amateur
Packet Address : VE3NJW@VE3KYT.#EON.ON.CAN
Freenet Address: aj467@Freenet.Carleton.ca
------------------------------
Date: (null)
From: (null)
SB DX ARL ARLD065
ARLD065 DX news
Documentation has been received and approved for the following
operations:
3D2UF operations beginning 20 November 1992
4J1FM operations beginning 21 October 1992
4J1FW operations beginning 21 October 1992
5W1VL operations beginning 25 November 1992
6O/FE1LVR operations beginning 18 January 1993
A61AF operations beginning 3 August 1993
C56V operations beginning 30 October 1993
C56/KF7AY operations beginning 28 Otober 1993
C56/AA7NO operations beginning 28 October 1993
C56/N7BG operations beginning 28 October 1993
KH2/N6SVL operations beginning 5 November 1993
KH6/N6SVL operations beginning 3 November 1993
V51/DJ2ZS operations beginning 17 August 1993
V51/DJ0WQ operations beginning 17 August 1993
V51/DK2WH operations beginning 21 July 1993
V63UF operations beginning 10 November 1993
V73UF operations beginning 17 November 1993
YA1AR operations beginning 5 December 1992
ZK1AUF operations beginning 17 November 1992
ZL/N6SVL operations beginning 11 November 1992
ZS9/DJ2ZS operations beginning 6 August 1993
ZS9/DJ0WQ operations beginning 6 August 1993
ZS0PI operations beginning 28 July 1993
NNNN
/EX
------------------------------
Date: Wed, 1 Dec 1993 09:46:07 GMT
From: swrinde!cs.utexas.edu!utnut!torn!nott!cunews!freenet.carleton.ca!Freenet.carleton.ca!aj467@network.ucsd.edu
To: info-hams@ucsd.edu
References <1993Nov30.153613.461@ke4zv.atl.ga.us>, <9311291536.AA28993@ocpfcad>, <CH9Jnp.F9v@freenet.carleton.ca>a
Reply-To : aj467@Freenet.carleton.ca (Bill Macpherson)
Subject : Re: expensive?
In a previous article, gary@ke4zv.atl.ga.us (Gary Coffman) says:
>In article <CH9Jnp.F9v@freenet.carleton.ca> aj467@Freenet.carleton.ca (Bill Macpherson) writes:
>>
>>I should have responded the first time ................. Bill
>>
>>>I was SHOCKED to see that the mainstay computer in packet
>>>was the commodore 64. I have one, collecting dusting my basement for
>>>years.
>>
>>I don't know why you're shocked to see the C=64 as a mainstay in Packet.
>>There is no need for wizz-bang horsepower, just to print little characters
>>to the screen.
>
>Indeed, an even cheaper approach is to use a dumb terminal or ASR33
>to work with the *Terminal* Node Controller since you don't have to
>tie up a TV set too, if all you need is to print little characters
>on a screen or paper. Of course if you want to take advantage of
>the more general features of packet, such as file and Email transfer,
>and if you want to take advantage of higher speeds, you'll dump the
>*Terminal* Node Controller and the clunky old display technology and
>adapt a DMA digital interface card in a more modern bus oriented
>computer running some competent networking software.
>
>>In fact it was innovation by some programmers in Germany
>>that brought us the Baycom TNC. If this isn't an application of high tech
>>( relatively speaking ) what is. It may be old, and not the latest technology,
>>but that in itself doesn't make it useless. If you want all the latest "
>>Bells and Whistles " Ham Radio can be expensive. If you want what works, and
>>are willing to expend some effort and/or elbow grease, Ham Radio can be
>>quite reasonable, while still being innovative.
>
>Baycom is a neat hack, though I wouldn't call it high tech, and it doesn't
>require a C64, IBM compatables work too. But it is a low speed solution
>oriented to squelched FM radios, and one that excessively ties up your
>computing resources counting zero crossings. It's satisfactory for the
>trivial terminal to terminal chat function on an otherwise unused computer,
>but that's a small part of what packet is capable of doing.
>
>Gary
>--
>Gary Coffman KE4ZV | Where my job's going, | gatech!wa4mei!ke4zv!gary
>Destructive Testing Systems | I don't know. It might | uunet!rsiatl!ke4zv!gary
>534 Shannon Way | wind up in Mexico. | emory!kd4nc!ke4zv!gary
>Lawrenceville, GA 30244 | -NAFTA Blues |
You almost caught me again eh!
I wasn't trying to suggest that the C=64 is the final answer to Packet,
merely that you don't have to have the biggest, fastest, most expensive
toys on the block to participate in Ham Radio.
With respect to the Baycom, it was developed ( hacked ) on the C=64, and
cloned/ported/ whatever to the IBM environment.
I wasn't trying to present the whole story. I was just trying to present
the "Frugal Gourmet/Urban Peasant" approach to Ham Radio. See I do watch
things besides ( yuck WWF ) and I'm not married to my sister either.
Just plain dumb old Bill
--
Bill VE3NJW Advanced Amateur
Packet Address : VE3NJW@VE3KYT.#EON.ON.CAN
Freenet Address: aj467@Freenet.Carleton.ca
------------------------------
Date: 1 Dec 1993 23:23:04 -0600
From: ucsnews!sol.ctr.columbia.edu!usc!cs.utexas.edu!geraldo.cc.utexas.edu!thumper.cc.utexas.edu!not-for-mail@network.ucsd.edu
To: info-hams@ucsd.edu
References <2cges6$agf@eis.ctp.org>, <2d95ndINNbvk@abc.ksu.ksu.edu>, <1993Nov30.145018.215@ke4zv.atl.ga.us>cc.utexa
Subject : Re: FT530 receiver problems??
Actually, there is a very simple solution to this problem which I just now
thought of. Why didn't I think of it before??
Is your AM detector on on your FT-530?
(Don't ask me about the display. I dunno.)
Tune to the offending signal (on frequency--not off) and press
F/M
0
F/m
# (or VFO whatever it's label is)
See if that don't clear it up.
73,
--
Buddy Brannan, KB5ELV | God is love.
Riff-Raff #4 | Love is blind.
Internet: | Buddy is blind.
davros@ccwf.cc.utexas.edu | Buddy is god.
------------------------------
End of Info-Hams Digest V93 #1419
******************************
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