home *** CD-ROM | disk | FTP | other *** search
Date: Sun, 28 Nov 93 01:10:50 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 #1395 To: Info-Hams Info-Hams Digest Sun, 28 Nov 93 Volume 93 : Issue 1395 Today's Topics: Calculating SWR Daily Summary of Solar Geophysical Activity for 20 November Daily Summary of Solar Geophysical Activity for 26 November Email callbook server (2 msgs) How useful are DSP units in noisy locations? Mag Mount Paint Damage Modem Software to Alert Many Pagers? 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: Sat, 27 Nov 1993 18:48:05 GMT From: yuma!galen@purdue.edu Subject: Calculating SWR To: info-hams@ucsd.edu In article <1993Nov26.200816.19512@combdyn.com> lawrence@combdyn.com (Lawrence *The Dreamer* Chen) writes: >How do you calculate SWR? I have a power meter...and I can measure the forward >and reflected power. How to I take the two values to determine the SWR? 1+SQRT(Wr/Wf) VSWR= _______________ 1-SQRT(Wr/Wf) Where SQRT denotes the square root of (this), Wr is reflected power and Wf is forward power. >Right now I have forward power of 5 Watts and reflected power of 0.1 Watts, >what SWR would that correspond to? I get 1.329:1 . Galen, KF0YJ ------------------------------ Date: Sat, 20 Nov 1993 21:55:55 MST From: dog.ee.lbl.gov!agate!usenet.ins.cwru.edu!magnus.acs.ohio-state.edu!math.ohio-state.edu!cyber2.cyberstore.ca!nntp.cs.ubc.ca!alberta!adec23!ve6mgs!usenet@network.ucsd.edu Subject: Daily Summary of Solar Geophysical Activity for 20 November To: info-hams@ucsd.edu /\/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\ DAILY SUMMARY OF SOLAR GEOPHYSICAL ACTIVITY 20 NOVEMBER, 1993 /\/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\ (Based In-Part On SESC Observational Data) SOLAR AND GEOPHYSICAL ACTIVITY INDICES FOR 20 NOVEMBER, 1993 ------------------------------------------------------------ !!BEGIN!! (1.0) S.T.D. Solar Geophysical Data Broadcast for DAY 324, 11/20/93 10.7 FLUX=100.5 90-AVG=094 SSN=058 BKI=3312 1221 BAI=007 BGND-XRAY=B1.5 FLU1=3.7E+05 FLU10=1.2E+04 PKI=3411 2222 PAI=009 BOU-DEV=021,026,006,012,009,010,010,007 DEV-AVG=012 NT SWF=00:000 XRAY-MAX= C5.2 @ 0032UT XRAY-MIN= B1.2 @ 1919UT XRAY-AVG= B4.0 NEUTN-MAX= +002% @ 0945UT NEUTN-MIN= -002% @ 1145UT NEUTN-AVG= -0.3% PCA-MAX= +0.1DB @ 1215UT PCA-MIN= -0.1DB @ 1900UT PCA-AVG= +0.0DB BOUTF-MAX=55364NT @ 0231UT BOUTF-MIN=55346NT @ 1952UT BOUTF-AVG=55355NT GOES7-MAX=P:+000NT@ 0000UT GOES7-MIN=N:+000NT@ 0000UT G7-AVG=+066,+000,+000 GOES6-MAX=P:+128NT@ 1836UT GOES6-MIN=N:-070NT@ 0951UT G6-AVG=+087,+019,-038 FLUXFCST=STD:105,110,110;SESC:105,110,110 BAI/PAI-FCST=010,010,020/012,015,035 KFCST=1115 4000 1112 2111 27DAY-AP=009,029 27DAY-KP=4222 1221 2235 6533 WARNINGS=*SWF ALERTS=**245STRM:0613-0817UTC !!END-DATA!! NOTE: The Effective Sunspot Number for 19 NOV 93 was 25.0. The Full Kp Indices for 19 NOV 93 are: 3+ 6- 2- 2o 3- 4- 3- 3o SYNOPSIS OF ACTIVITY -------------------- Solar activity was low. Region 7618 (N07W31) remains the most impressive area on the disk. In white light, the region has decreased in area and spot number, but still retains its beta-delta configuration. New Region 7621 (S09E48) was numbered overnight. An area of interest to watch is on the east limb at N12 where an impressive bright surge was reported by Learmonth last night. All other areas/regions were stable. Solar activity forecast: solar activity is expected to be low to moderate with Region 7618 the most likely candidate to produce C and M-class activity. A new, active region may rotate into view over the next few days and could also contribute to activity. STD: X-ray imagery from the Yohkoh satellite showed a fairly strong and bright loop system at about 02:50 UTC from the region just beyond the east limb. A Yohkoh full-disk x-ray image showing the enhanced northeast limb emissions has been appended to this report. The geomagnetic field has been at mostly unsettled levels. Since 09Z, the middle latitude field has been at quiet levels. Geophysical activity forecast: the geomagnetic field is expected to be at mostly unsettled levels for the first two days of the period with active to minor storm conditions expected early on day three due to a favorably located coronal hole. The disturbance is expected to last only one day with levels forecasted to decrease to mostly unsettled thereafter. Event probabilities 21 nov-23 nov Class M 50/50/50 Class X 05/05/05 Proton 05/05/05 PCAF Green Geomagnetic activity probabilities 21 nov-23 nov A. Middle Latitudes Active 20/25/35 Minor Storm 10/10/20 Major-Severe Storm 01/05/10 B. High Latitudes Active 25/30/40 Minor Storm 10/15/30 Major-Severe Storm 01/10/15 HF propagation conditions were near-normal over the low and middle latitude paths. High and polar latitude paths experienced additional periods of below-normal propagation due primarily to periods of enhanced geomagnetic and auroral activity within the auroral zone. Conditions improved notably by the end of the day. Propagation conditions are expected to continue near-normal over the next 48 hours (through about 22 November inclusive). Activity could become gradually enhanced during the latter half of 22 November. On 23 November, a recurrent coronal hole is expected to increase levels of geophysical activity to near-storm levels which is expected to cause below-normal (poor to occasionally very poor) propagation for transpolar and transauroral paths. Middle-latitude night-sector paths may also be affected on 22 November. COPIES OF JOINT USAF/NOAA SESC SOLAR GEOPHYSICAL REPORTS ======================================================== REGIONS WITH SUNSPOTS. LOCATIONS VALID AT 20/2400Z NOVEMBER ----------------------------------------------------------- NMBR LOCATION LO AREA Z LL NN MAG TYPE 7618 N08W31 338 0580 DKI 08 026 BETA-DELTA 7620 N04E43 264 0000 AXX 01 001 ALPHA 7621 S10E49 258 0000 AXX 00 001 ALPHA REGIONS DUE TO RETURN 21 NOVEMBER TO 23 NOVEMBER NMBR LAT LO NONE LISTING OF SOLAR ENERGETIC EVENTS FOR 20 NOVEMBER, 1993 ------------------------------------------------------- BEGIN MAX END RGN LOC XRAY OP 245MHZ 10CM SWEEP SWF NO EVENTS OBSERVED POSSIBLE CORONAL MASS EJECTION EVENTS FOR 20 NOVEMBER, 1993 ----------------------------------------------------------- BEGIN MAX END LOCATION TYPE SIZE DUR II IV 20/ 0338 0403 0444 N08W20 LDE C1.3 66 INFERRED CORONAL HOLES. LOCATIONS VALID AT 20/2400Z --------------------------------------------------- ISOLATED HOLES AND POLAR EXTENSIONS EAST SOUTH WEST NORTH CAR TYPE POL AREA OBSN 48 S42W53 S44W61 S09W90 S09W90 023 ISO NEG 010 10830A 49 N30E05 N18W04 N25W13 N38W05 316 ISO POS 005 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 ------ ---- ---- ---- ---- -- ------ ------ --------- --------- --------- 19 Nov: 0337 0342 0344 B3.1 SF 7618 N09W07 0359 0404 0408 B3.2 0710 0759 0828 B8.9 1845 2004 2051 B9.8 B2007 U2009 A2015 SF 7618 N12W12 REGION FLARE STATISTICS FOR THE PREVIOUS UTC DAY ------------------------------------------------ C M X S 1 2 3 4 Total (%) -- -- -- -- -- -- -- -- --- ------ Region 7618: 0 0 0 2 0 0 0 0 002 (40.0) Uncorrellated: 0 0 0 0 0 0 0 0 003 (60.0) Total Events: 005 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 =========================================================================== 20 November 1993, 02:50 UTC North .. . . . ..... ................ .................. .,,,,,,,,......,,:::::::::,:,,,...... .....,...,,,,,,::,,,,,..,.. .,,,,,,,,,,,,,,:::::::::;;::::,,,,..... .,,,,::,,,,,:::::;;;:,,,... ..........,.,,,,,,,,,,,,,,,:,::;;;;::,,,..... ,,::::;::::::::;;;;:::,.. ... ..........,,,,,,,,,,,,,.,,,,,,,:::::::,,,.... ::::;;;;;;;;;;;;;::::::,...... ...,,,,:,,,,,,,,,:,,,,,,,,,,,::;;;:::,,,,..... :;;;----------;::::,,::,,,..... .,.,,::::::::::::::::,,,,,,,,:::;;;;;:::,,,,.. ;;--+++++|++-;:::,,,::,,,,.. . . ....,:::;;;;---;;;;::,:,,,:,:::::;--;;;::,,,. ;--++||||||-;;:::;:,,,,,,... ...., . ..,::;;-+++++---;;:::::::::;:;:;-+-;;;::,, -+++|!111!+-;;;;::::,,,,,,............,,,,:;-+|!!!|++---;;;;;;;;;;;;;;-+--;:::, |!124*##4|+--;;;:::::,,,,.,:,,,,,,,,.,,,:+!!+;-!221!!|----;;;;;;;---;;;---;;;:: 13*@@@@@4|+----;;;:::,,,,,,,,,,,,,,,,,::::;+-;;-1432!!|++---;;;;;;;;;;;;+++-;;: 4*#@@@@@1|++----;-;:::,,,,,,,,,,,,,:::::::;;;;--!24**32++++--;;;;--;;;;;+!|+-;; 123*#@@3!!!|||--;;;;:,,,,,.,,,,,,,,--:::::::;;-+!4@@@*!|++----;;-++--;;;-||+--; ||!1233|||2!3+-;;;;;:,,,,,,,,,,,,,,,,,,,::::;-++|1#@#2|+-------;--------+||++-- --+++||---++-;::::;;:,,,,,,:,,,,,,,,,,,,,,::;-+|!112!|+------;;;;;;;;--+-|++--- ;;;----;;;;;;::::,:::,,,,,,,,,,,,,,,,,,,,,::;;-+||||||+;;;;--;;;-----+---+++--; :;;;---;;;+-:::::::::,,,,,,,,,,,,,,,,,,,.,:::::;;-;;;;;;;-;;;;----++||+--++--;; :::;;;--:;+|::::;;:,,::,::,,.,,,,:,,.,,,.,,,,,,:::::;;-+-;;;;----;-+||-;+|+-;;; ,:::;;;-;:::,:,,,,,,,,,,,,,,..,,,,:::,,......,,,,,,:::;;;::::;-;;-+|+;:-||+-;;; ,,::;;;;-;::,,,,,,,,,,,,,,,,.,,,,,,,,,,,.....,..,,,,:;;:::::;;----;:,:;||+--;;: ,,:::;;;;-;::,,,,,,,,,,,,,,,,,,,,,,............,,,,,,,,:;;;;;;;;::,,:;||++-;;;: .,,,::;;;;-;:;::::,,,,,,,,,,,,,,,..............,,,,,,,:,:::;;;;:,,,:-++++--;;:: ..,,,::::;;;--:::::,,,....,,.,...,...............,,,,,,,,::::::,,:;+++---;;;::, ...,,,:::::;;;;;::,,,,,,,,,,,,,,,........... . ..,,,,,..,,,....,;-----;;:::,,, ....,,,,:::;;;--;::,,,,,,.,,,,,......... .... .. ..,.,;;;;;;;:::,,,,.. .....,,,:::;;;;;::.... ..,,..... .......:;-;;;:::::,,,,..... ........,,,,:::::::,, . . . .,:;----;::::::,,,..... . .......,,,,,,,,,,,,,... ..,:;;----;;;;::::,,,,... ..............,,,................,,,::::;;;;;:::::::,,,,.... .. .. .. ... . ...,,,,,,,,,,,,.... ........... 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: Fri, 26 Nov 1993 20:54:14 MST From: swrinde!cs.utexas.edu!uwm.edu!spool.mu.edu!agate!library.ucla.edu!news.mic.ucla.edu!unixg.ubc.ca!kakwa.ucs.ualberta.ca!alberta!ugc!nebulus!ve6mgs!usenet@network.ucsd.edu Subject: Daily Summary of Solar Geophysical Activity for 26 November To: info-hams@ucsd.edu /\/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\ DAILY SUMMARY OF SOLAR GEOPHYSICAL ACTIVITY 26 NOVEMBER, 1993 /\/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\ (Based In-Part On SESC Observational Data) SOLAR AND GEOPHYSICAL ACTIVITY INDICES FOR 26 NOVEMBER, 1993 ------------------------------------------------------------ !!BEGIN!! (1.0) S.T.D. Solar Geophysical Data Broadcast for DAY 330, 11/26/93 10.7 FLUX=093.2 90-AVG=094 SSN=052 BKI=2222 2242 BAI=009 BGND-XRAY=B1.5 FLU1=9.2E+05 FLU10=1.3E+04 PKI=2212 2342 PAI=009 BOU-DEV=018,012,013,010,015,018,043,017 DEV-AVG=018 NT SWF=00:000 XRAY-MAX= C2.1 @ 1606UT XRAY-MIN= B1.3 @ 2328UT XRAY-AVG= B2.3 NEUTN-MAX= +002% @ 2155UT NEUTN-MIN= -002% @ 1810UT NEUTN-AVG= -0.1% PCA-MAX= +0.2DB @ 1545UT PCA-MIN= -0.3DB @ 2135UT PCA-AVG= +0.1DB BOUTF-MAX=55364NT @ 1344UT BOUTF-MIN=55333NT @ 1826UT BOUTF-AVG=55357NT GOES7-MAX=P:+000NT@ 0000UT GOES7-MIN=N:+000NT@ 0000UT G7-AVG=+064,+000,+000 GOES6-MAX=P:+130NT@ 1742UT GOES6-MIN=N:-055NT@ 0825UT G6-AVG=+085,+016,-028 FLUXFCST=STD:095,090,090;SESC:095,090,090 BAI/PAI-FCST=005,005,005/010,010,010 KFCST=3122 2112 3212 2122 27DAY-AP=005,007 27DAY-KP=2121 2122 1132 2223 WARNINGS=*SWF ALERTS= !!END-DATA!! NOTE: The Effective Sunspot Number for 25 NOV 93 was 42.0. The Full Kp Indices for 25 NOV 93 are: 2- 1+ 1o 0+ 2- 2o 2- 3- SYNOPSIS OF ACTIVITY -------------------- Solar activity was low with several C-class flares observed. New Region 7623 (S11E67) rotated onto the disk and produced a C2/SF flare at 26/1605Z. Region 7620 (N04W40) produced a C1 flare at 26/1712Z. All regions appear to be stable. Solar activity forecast: solar activity is expected to be at low levels during the period. STD: The latest Yohkoh image has been appended to this report. The geomagnetic field has been at quiet levels for the past 24 hours. High latitudes reported isolated undettled levels during the period. Geophysical activity forecast: the geomagnetic field is expected to be at quiet to unsettled levels. Event probabilities 27 nov-29 nov Class M 10/10/10 Class X 01/01/01 Proton 01/01/01 PCAF Green Geomagnetic activity probabilities 27 nov-29 nov A. Middle Latitudes Active 05/05/05 Minor Storm 05/05/05 Major-Severe Storm 01/01/01 B. High Latitudes Active 05/05/10 Minor Storm 01/05/05 Major-Severe Storm 01/01/01 HF propagation conditions were normal over all regions. No changes are expected over the next three days, through 29 November inclusive. Normal propagation should persist over all regions. COPIES OF JOINT USAF/NOAA SESC SOLAR GEOPHYSICAL REPORTS ======================================================== REGIONS WITH SUNSPOTS. LOCATIONS VALID AT 26/2400Z NOVEMBER ----------------------------------------------------------- NMBR LOCATION LO AREA Z LL NN MAG TYPE 7620 N04W40 268 0280 ESI 12 017 BETA 7622 N13E06 222 0040 CSO 03 004 BETA 7623 S11E67 161 0030 HAX 01 001 ALPHA 7621 S09W30 258 PLAGE REGIONS DUE TO RETURN 27 NOVEMBER TO 29 NOVEMBER NMBR LAT LO NONE LISTING OF SOLAR ENERGETIC EVENTS FOR 26 NOVEMBER, 1993 ------------------------------------------------------- BEGIN MAX END RGN LOC XRAY OP 245MHZ 10CM SWEEP NONE POSSIBLE CORONAL MASS EJECTION EVENTS FOR 26 NOVEMBER, 1993 ----------------------------------------------------------- BEGIN MAX END LOCATION TYPE SIZE DUR II IV NO EVENTS OBSERVED INFERRED CORONAL HOLES. LOCATIONS VALID AT 26/2400Z --------------------------------------------------- ISOLATED HOLES AND POLAR EXTENSIONS EAST SOUTH WEST NORTH CAR TYPE POL AREA OBSN 51 S01E47 S13E32 N15E15 N35E42 202 ISO POS 023 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 ------ ---- ---- ---- ---- -- ------ ------ --------- --------- --------- 25 Nov: 0009 0020 0037 C1.0 SF 7620 N04W14 0105 0105 0112 SF 7620 N05W14 0116 0117 0124 SF 7620 N03W15 0138 0145 0204 B9.7 SF 7620 N05W14 0343 0357 0406 C2.6 0458 0518 0527 SF 7620 N03W15 0534 0540 0555 C1.2 1N 7620 N03W17 0614 0621 0625 C5.7 0805 0809 0815 C2.1 SF 7620 N03W17 0902 0912 0918 C1.9 SF 7620 N04W19 1214 1223 1231 B7.5 1744 1754 1803 B3.9 2020 2027 2037 C1.8 SF 7620 N04W24 2251 2254 2256 B2.7 REGION FLARE STATISTICS FOR THE PREVIOUS UTC DAY ------------------------------------------------ C M X S 1 2 3 4 Total (%) -- -- -- -- -- -- -- -- --- ------ Region 7620: 5 0 0 8 1 0 0 0 009 (64.3) Uncorrellated: 2 0 0 0 0 0 0 0 005 (35.7) Total Events: 014 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 ------ ---- ---- ---- ---- -- ------ ------ --------------------------- 25 Nov: 0614 0621 0625 C5.7 III 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 =========================================================================== 26 November 1993, 02:00 UTC North . ................. . ....,...,.......... .....,:,:,,,,,,,,,...... .....,.,,,,,,,,,,,,,,,.,........,,:::::::,,,,..... .... .........,,.,,,,,,,,,,,,,,,,,,,,,,,..,...,,,::::::,,,,,....... .......,,,,,,. ....,,,,,,,,,,,,,,,,,,,,,,,,,,,,,,,,...,,:;::::,,,,,,,.... .....,,,::::,.. ...,,,:,,,,,,,,,,,,,,,,,,,,,,,,,,,,,,,,,..,:;;:::::::,,,,. ...,,,,,:-+-:;:,......,::::::::::,,,::,,,,,,,,,,,,,,,,,,,,,,,,,,,:;;--;;;;:::, ..,,,,:::-|!|;:,,... ..,::;;:;;::::::::::::,,,,,,,,,,,,,,:,,:::::,,:-++++++--;: ,,:::::;;-|21-:,... ...,,:;;-------;::::::::,:,,,:,,,,,,,,,,,::::::::+!!||+-;;: .,::;;;;;;;-;:.. .....,,,:;---+||+++-;;::::::::,:,::,:,:::::::::::::::+!!!|-;;: ,,:::;;;:,,... ....,,,::;+++|!!|+++-;;;;;::::::;;;;;:;;::::::::::::;!21+-;;; ,,::;;;;,.. .. ....,,,,,:;-4331!!||++---;;;;;;;;;;;;---+++-;:::::::;:;-221!||+ ,::;;;-;,. . ...,,,,::::;;|21!|||++++-----;--++-----+|!!|+|-;;::::::;;-3*31||| ::;;---;,. .. ..,,,,:,,::;;--------;;::;;;;;--++++--+|24*3!++-;;:::::;;+1#3!+-- ;;--+++-:.......,,,,,,,::;;;;;;;;;;;;:;;::::;-++++--+3@@@3!++-;::::::;;-|431!+; ;--+|!!-:.......,,,,,,,,::::::::::::::::::,::;;;;;;-+!122!!-;;;:::,::::;-|!|+-; -+|!122|:,,,...,,,,,:,,,,,,,,,,,,::,,,,,,,,,,::::;;;-||||!|;::::::,:::;;-+--;;: -++!123!-;;:;:,,,:::::,,,,,,,,,,,,,,,,,,,,,,,,::;;;:;;;---;;::,,,,,::::;--;;:,, ;-++!122|+--++:,:::::,,,,,,,,,,,,,,,,,,,,....,:::-+:,:::::::,,,,,,,,,::;-;::,,, ;;;+|!11!+++||-;;;::,,,,,,,,..,.,.,,.,........,,,:,,,,,,,,,,,,,,,,,,:::-;:,,,,, ::;++|!!|++!1!-;;;::,,,....................,...,........,,,,,,,,,,,,::;;:,,,... .,;;----++---;;-;;::,,,................................,,,,,,,,,,,,,:;;::,,.... .,::;;;------;;;;::::,,,.,,.,,................,...,,,,,,,,,,,,,,,,,:;;::,,..... .,,:::;;;-----;:::,,,,,,,........................,,,,,,,....,.,,,:::::,,,..... .,,,::::;;;;;;;;::,,,,,,......................,..........,,,,,,,::,,,,.... ..,,,,:::::::;;;;;::,,,.......,,,..,,...,...,,,,,,,,,,,,,,,,,,,,,.... ...,,,,,,::::;;;;;;;:,,,... . .........,...............,,,... .....,,,,,::::;;;-----;;:,. . ... .......,,,,,::;;;;;;;;;;::,.. ... .......,,,,,,,:::::,,,... ......... ................... .. 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: 28 Nov 93 06:24:50 GMT From: ogicse!uwm.edu!cs.utexas.edu!howland.reston.ans.net!noc.near.net!news.delphi.com!usenet@network.ucsd.edu Subject: Email callbook server To: info-hams@ucsd.edu In the last message I said that he (ko4rk, aka 44.62.0.122) might not pick up an Internet message from an .ampr. source. That should have read a NON-.ampr. source, that is, not from a packet BBS. Also, there are other REQQTH servers all over the place. This is the only one I am sure of. Again, hope this helps. Jason! ------------------------------ Date: 28 Nov 93 06:19:52 GMT From: ogicse!uwm.edu!cs.utexas.edu!howland.reston.ans.net!noc.near.net!news.delphi.com!usenet@network.ucsd.edu Subject: Email callbook server To: info-hams@ucsd.edu The only E-mail servers I know of are available on packet BBSs. You may want to try the following (It might work): send a message to REQQTH@44.62.0.122 and in the SUBJECT of the message, put the callsign(s) of the station(s) you are looking for, separated only by spaces. Put nothing in the actual text section. I'm not sure if he will pick up an Internet message from a .ampr. source, but it might be worth a shot. You might also try a telnet to plan9.njit.edu 2000 or mudgate.imsa.edu 2000. I hope I've answered your question with at least one of the options. -=*>Jason!<*=- JTRIOLO@delphi.com kd4acg@k9iu.ampr.org (k9iu.#sin.in.usa.na) kd4acg@wa4ong.ampr.org (wa4ong.va.usa.na) ------------------------------ Date: 25 Nov 1993 16:22:58 GMT From: munnari.oz.au!sgiblab!swrinde!gatech!usenet.ufl.edu!mailer.acns.fsu.edu!freenet2.scri.fsu.edu!friederw@network.ucsd.edu Subject: How useful are DSP units in noisy locations? To: info-hams@ucsd.edu NIR-10 does a really good job for me here in Tallahassee. The recent firmware upgrade did wonders for it--QRN almost disappears! 73 -- ********************************************************************************************** William A. "Bill" Frieder friederw@freenet.tlh.fl.us N4QNF Packet Mail = N4QNF @ W1FJI (904) 488-2381 days (904) 893-3738 till 9:30 P.M. EDT ------------------------------ Date: Fri, 26 Nov 1993 21:49:00 GMT From: pacbell.com!UB.com!wetware!rhohan!express@ames.arpa Subject: Mag Mount Paint Damage To: info-hams@ucsd.edu SMK>From: sknapp@iastate.edu (Steven M. Knapp) SMK>Organization: Iowa State University, Ames, IA SMK>In article <CGx7KB.FHq@srgenprp.sr.hp.com> alanb@sr.hp.com (Alan SMK>Bloom) writes: SMK>>David Van Nuys (vannuysd@sonoma.edu) wrote: SMK>>: I notice that my two-meter mag mount is leaving rings on the paint SMK>of my SMK>>: trunk. Has anyone got any tips for preserving the paint and still SMK>using SMK>>: a mag mount? Try putting the base of the antenna into a plastic sandwich bag and e car. Steve Fleckenstein - Red Onion Express BBS - 914-342-4585 * OLX 2.1 TD * Paper clips are the larval stage of coat hangers. --- RBBSMail v18.2 * Origin: Red Onion, Express Wawayanda,New York 914 342 4585 (100:911/7.0) ------------------------------ Date: 22 Nov 1993 03:05:00 GMT From: dog.ee.lbl.gov!agate!howland.reston.ans.net!cs.utexas.edu!geraldo.cc.utexas.edu!slip-3-1.ots.utexas.edu!user@network.ucsd.edu Subject: Modem Software to Alert Many Pagers? To: info-hams@ucsd.edu Our local Amateur Radio Emergency Service (ARES) group needs some software that could notify all our pager-carrying members when an emergency happens. Many of our members carry pagers for their jobs, and most of these are digital pagers. We need an application that would go down a list of pager phone numbers, dialing each, waiting until the phone is answered, then sending the TouchTones (r) for "14694". This number would be recognized by our members as meaning 146.94 MHz, the local ARES repeater frequency. Has anyone seen an app (for PC or Mac) that can do this? Thank you. = = = = = = = = = = = = = = = = = = = = _ Miles Abernathy, N5KOB = | |__ miles@mbs.telesys.utexas.edu = _| | POB 7580, Austin TX 78713 = \ * / University of Texas @ Austin = \/ tel. (512) 471-6521 U.S.A. = = = = = = = = = = = = = = = = = = = = = ------------------------------ End of Info-Hams Digest V93 #1395 ****************************** ****************************** 
