Date: Thu, 12 May 94 04:30:06 PDT From: Info-Hams Mailing List and Newsgroup Errors-To: Info-Hams-Errors@UCSD.Edu Reply-To: Info-Hams@UCSD.Edu Precedence: Bulk Subject: Info-Hams Digest V94 #515 To: Info-Hams Info-Hams Digest Thu, 12 May 94 Volume 94 : Issue 515 Today's Topics: << Looking for Ham cdrom disk for BBS >> Daily Summary of Solar Geophysical Activity for 09 May Send Replies or notes for publication to: Send subscription requests to: 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: Tue, 10 May 1994 03:50:33 GMT From: lerc.nasa.gov!kira.cc.uakron.edu!malgudi.oar.net!witch!doghouse!jsalemi@purdue.edu Subject: << Looking for Ham cdrom disk for BBS >> To: info-hams@ucsd.edu In article <>, Guy Quenneville (guy@penage.CS.laurentian.CA) writes: > I'm looking for a CDROM disk that can be used in a BBS that is >Ham related. I have heard of the BUCKMASTER cdrom but I know nothing else >about it. Could someone please help, Thanks > I run the Buckmaster on my LL BBS. Call 703-548-7849 to check it out. Works great, and it's the only CD-ROM out there that has a bunch of international calls in addition to the US and Canada. 73...joe ---------- Joe Salemi, KR4CZ Internet: jsalemi@doghouse.win.net Compuserve: 72631,23 FidoNet: 1:109/136 MCI Mail: 433-3961 ------------------------------ Date: Mon, 9 May 1994 23:30:27 MDT From: ihnp4.ucsd.edu!galaxy.ucr.edu!library.ucla.edu!psgrain!nntp.cs.ubc.ca!alberta!ve6mgs!usenet@network.ucsd.edu Subject: Daily Summary of Solar Geophysical Activity for 09 May To: info-hams@ucsd.edu /\/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\ DAILY SUMMARY OF SOLAR GEOPHYSICAL ACTIVITY 09 MAY, 1994 /\/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\ (Based In-Part On SESC Observational Data) SOLAR AND GEOPHYSICAL ACTIVITY INDICES FOR 09 MAY, 1994 ------------------------------------------------------- !!BEGIN!! (1.0) S.T.D. Solar Geophysical Data Broadcast for DAY 129, 05/09/94 10.7 FLUX=077.3 90-AVG=087 SSN=016 BKI=4634 3333 BAI=026 BGND-XRAY=A3.7 FLU1=3.2E+06 FLU10=1.4E+04 PKI=4545 3333 PAI=024 BOU-DEV=050,120,038,049,027,034,029,031 DEV-AVG=047 NT SWF=00:000 XRAY-MAX= B1.0 @ 1126UT XRAY-MIN= A2.5 @ 1947UT XRAY-AVG= A6.2 NEUTN-MAX= +003% @ 1610UT NEUTN-MIN= -002% @ 1925UT NEUTN-AVG= -0.1% PCA-MAX= +0.1DB @ 2240UT PCA-MIN= -0.2DB @ 0350UT PCA-AVG= +0.0DB BOUTF-MAX=55348NT @ 0319UT BOUTF-MIN=55301NT @ 1101UT BOUTF-AVG=55320NT GOES7-MAX=P:+000NT@ 0000UT GOES7-MIN=N:+000NT@ 0000UT G7-AVG=+081,+000,+000 GOES6-MAX=P:+134NT@ 1829UT GOES6-MIN=N:-105NT@ 0306UT G6-AVG=+101,+030,-040 FLUXFCST=STD:078,080,081;SESC:078,080,081 BAI/PAI-FCST=020,020,020/025,025,020 KFCST=3434 4334 4435 4334 27DAY-AP=025,025 27DAY-KP=5553 3344 3454 3444 WARNINGS=*GSTRM;*AURMIDWCH ALERTS= !!END-DATA!! NOTE: The Effective Sunspot Number for 08 MAY 94 was 13.9. The Full Kp Indices for 08 MAY 94 are: 5- 5o 6o 5- 4- 3+ 4- 4o The 3-Hr Ap Indices for 08 MAY 94 are: 38 50 78 41 22 19 25 29 Greater than 2 MeV Electron Fluence for 09 MAY is: 2.2E+09 SYNOPSIS OF ACTIVITY -------------------- Solar activity was very low. No events were observed the past 24 hours. Region 7719 (S06W01), the only spotted region on the disk, is in slow decay. Solar activity forecast: solar activity is expected to be very low. The geomagnetic field has been at unsettled to major storm levels for the past 24 hours. The GT 2 MeV electron flux remained very high. Geophysical activity forecast: the geomagnetic field is expected to be mostly unsettled to active with periods of local nighttime minor storm conditions expected. Event probabilities 10 may-12 may Class M 01/01/01 Class X 01/01/01 Proton 01/01/01 PCAF Green Geomagnetic activity probabilities 10 may-12 may A. Middle Latitudes Active 20/20/30 Minor Storm 35/35/20 Major-Severe Storm 05/05/05 B. High Latitudes Active 25/25/25 Minor Storm 40/40/35 Major-Severe Storm 10/10/05 HF propagation conditions were below-normal over most regions today, particularly high-latitude southern-hemisphere night-sector paths where occassional significant degradation was reported with MUF depressions approaching 50% of normal. Daytime conditions were not as heavily depressed. No significant changes are foreseen for the next 48 to 72 hours. A very gradual improvement is still expected, but will likely be frequently intermixed with degraded periods. COPIES OF JOINT USAF/NOAA SESC SOLAR GEOPHYSICAL REPORTS ======================================================== REGIONS WITH SUNSPOTS. LOCATIONS VALID AT 09/2400Z MAY ------------------------------------------------------ NMBR LOCATION LO AREA Z LL NN MAG TYPE 7719 S06W03 229 0020 CSO 06 006 BETA 7713 N06W67 293 PLAGE 7714 S14W58 284 PLAGE 7718 N10W12 238 PLAGE 7720 S10E25 201 PLAGE REGIONS DUE TO RETURN 10 MAY TO 12 MAY NMBR LAT LO 7708 N09 109 7701 N07 120 LISTING OF SOLAR ENERGETIC EVENTS FOR 09 MAY, 1994 -------------------------------------------------- BEGIN MAX END RGN LOC XRAY OP 245MHZ 10CM SWEEP NONE POSSIBLE CORONAL MASS EJECTION EVENTS FOR 09 MAY, 1994 ------------------------------------------------------ BEGIN MAX END LOCATION TYPE SIZE DUR II IV 09/B1511 B1543 N03W90 EPL INFERRED CORONAL HOLES. LOCATIONS VALID AT 09/2400Z --------------------------------------------------- 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 ------ ---- ---- ---- ---- -- ------ ------ --------- --------- --------- NO EVENTS OBSERVED. 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 0 000 ( 0.0) Total Events: 000 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: Wed, 11 May 1994 17:14:01 GMT From: ihnp4.ucsd.edu!dog.ee.lbl.gov!agate!howland.reston.ans.net!gatech!newsfeed.pitt.edu!ctc.com!news.mic.ucla.edu!library.ucla.edu!csulb.edu!csus.edu!netcom.com!dgf@network.ucsd.edu To: info-hams@ucsd.edu References <2qm2fp$47@tuba.cit.cornell.edu>, <1994May11.035124.12133@ke4zv.atl.ga.us>, <2qqmij$t5q@sol.sun.csd.unb.ca>com Subject : Re: use INTERNET for linked repeater? In article <2qqmij$t5q@sol.sun.csd.unb.ca> a4q4@jupiter.sun.csd.unb.ca (D.J.Trynor EE) writes: > I would imagine something of that sort would have to be done using >a buffer to store the voice data and sent all at once, in the same fashion >as a simplex repeater operates. The rise and fall of network traffic would >make for a choppy converstaion if it were done real time. > >Sounds like a good idea none the less... > >Don There is a program mentioned in the linux area called "atalk" which takes incoming audio to a soundblaster card and transmits it through an internet connection to another location (anyway, this was my understanding). I think it would be limited somewhat by the current speed of dial-in connections (14kbps) and the lousy throughput of most internet service providers (including this one). 73 Dave WB0GAZ dgf@netcom.com ------------------------------ End of Info-Hams Digest V94 #515 ******************************