LDR | |
03055cam a2200529Ii 4500 |
001 |
|
102198683 |
003 |
|
MiAaHDL |
005 |
|
20220727000000.0 |
006 |
|
m d |
007 |
|
cr bn ---auaua |
008 |
|
090515e197612 maua bt f000 0 eng d |
035 |
⊔ |
⊔ |
‡a(MiU)990157505590106381
|
035 |
⊔ |
⊔ |
‡asdr-miu.990157505590106381
|
035 |
⊔ |
⊔ |
‡z(MiU)MIU01000000000000015750559-goog
|
035 |
⊔ |
⊔ |
‡a(OCoLC)321045302
|
035 |
⊔ |
⊔ |
‡z(MiU)Aleph015750559
|
040 |
⊔ |
⊔ |
‡aLHL
‡beng
‡cLHL
‡dOCLCF
‡dOCLCO
‡dOCLCQ
‡dCOD
‡dTRAAL
|
049 |
⊔ |
⊔ |
‡aMAIN
|
086 |
0 |
⊔ |
‡aD 301.45/39:585
|
088 |
⊔ |
⊔ |
‡aADA 038782
|
088 |
⊔ |
⊔ |
‡aAFGL TR 76-295
|
100 |
1 |
⊔ |
‡aGuidice, Donald A.
|
245 |
1 |
0 |
‡aPolarization spectra of centimeter-wavelength solar bursts using whole-sun observations /
‡cDonald A. Guidice.
|
264 |
⊔ |
1 |
‡aHanscom AFB, Massachusetts :
‡bAir Force Geophysics Laboratories, Air Force Systems Command, United States Air Force,
‡c1976.
|
300 |
⊔ |
⊔ |
‡a36 pages :
‡billustrations ;
‡c28 cm.
|
336 |
⊔ |
⊔ |
‡atext
‡btxt
‡2rdacontent
|
337 |
⊔ |
⊔ |
‡aunmediated
‡bn
‡2rdamedia
|
338 |
⊔ |
⊔ |
‡avolume
‡bnc
‡2rdacarrier
|
490 |
0 |
⊔ |
‡aAFGL-TR ;
‡v76-295
|
490 |
0 |
⊔ |
‡aEnvironmental Research Papers ;
‡vNo. 585
|
500 |
⊔ |
⊔ |
‡aResearch supported by the Air Force Geophysics Laboratory, Air Force Systems Command, United States Air Force, Hanscom AFB, Massachusetts.
|
500 |
⊔ |
⊔ |
‡aSpace Physics Division Project 4643.
|
500 |
⊔ |
⊔ |
‡aADA038782 (from http://www.dtic.mil).
|
500 |
⊔ |
⊔ |
‡a"8 December 1976."
|
504 |
⊔ |
⊔ |
‡aIncludes bibliographical references (pages 35-36).
|
520 |
⊔ |
⊔ |
‡aThe physics of microwave-burst emission is briefly examined to give the rationale for investigating polarization spectra. The instruments used to carry out the 9.4 GHz and 7 GHz circular-polarization measurements and the 5 GHz Stokes-parameter measurements are described. A survey of the August 1972 to December 1973 period produced a table of 45 bursts, from which some limited results were obtained. About 75 to 80 percent of all bursts are circularly polarized, with varying polarization over the 5 to 9.4 GHz range. For most bursts where the circular polarization pc increases toward the upper or lower end of the 5 to 9.4 GHz range, the total intensity I also increases in that direction. The few bursts having a pc sense reversal in the 5 to 9.4 GHz range also have a spectral maximum of I at roughly the same frequency. Some simplified explanations of the results are presented.
|
538 |
⊔ |
⊔ |
‡aMode of access: Internet.
|
650 |
⊔ |
7 |
‡aSpectrum, Solar.
‡2fast
‡0(OCoLC)fst01129134
|
650 |
⊔ |
7 |
‡aSolar radiation.
‡2fast
‡0(OCoLC)fst01125164
|
650 |
⊔ |
7 |
‡aSolar activity.
‡2fast
‡0(OCoLC)fst01124887
|
650 |
⊔ |
7 |
‡aRadio waves.
‡2fast
‡0(OCoLC)fst01087617
|
650 |
⊔ |
7 |
‡aRadio astronomy.
‡2fast
‡0(OCoLC)fst01087196
|
650 |
⊔ |
7 |
‡aElectromagnetic waves
‡xPolarization.
‡2fast
‡0(OCoLC)fst00906583
|
650 |
⊔ |
0 |
‡aRadio astronomy.
|
650 |
⊔ |
0 |
‡aElectromagnetic waves
‡xPolarization.
|
650 |
⊔ |
0 |
‡aRadio waves.
|
650 |
⊔ |
0 |
‡aSpectrum, Solar.
|
650 |
⊔ |
0 |
‡aSolar activity.
|
650 |
⊔ |
0 |
‡aSolar radiation.
|
710 |
2 |
⊔ |
‡aU.S. Air Force Geophysics Laboratory.
|
730 |
0 |
⊔ |
‡aTechnical Report Archive & Image Library (TRAIL)
|
899 |
⊔ |
⊔ |
‡a39015095136225
|
CID |
⊔ |
⊔ |
‡a102198683
|
DAT |
0 |
⊔ |
‡b20220727000000.0
|
DAT |
1 |
⊔ |
‡a20220728140741.0
‡b2024-04-23T17:34:02Z
|
CAT |
⊔ |
⊔ |
‡aSDR-MIU
‡dALMA
‡lprepare.pl-004-008
|
FMT |
⊔ |
⊔ |
‡aBK
|
HOL |
⊔ |
⊔ |
‡0sdr-miu.990157505590106381
‡aMiU
‡bSDR
‡cGWLA
‡pmdp.39015095136225
‡sMIU
‡1990157505590106381
|
974 |
⊔ |
⊔ |
‡bMIU
‡cGWLA
‡d20240423
‡sgoogle
‡umdp.39015095136225
‡y1976
‡rpd
‡qbib
‡tUS fed doc
|