FINE-STRUCTURE OF A VERY BRIGHT ACTIVE REGION AT A WAVELENGTH OF 2.8CM

被引：7

作者：

FELLI, M ^{[1
]}

PAMPALONI, P ^{[1
]}

TOFANI, G ^{[1
]}

机构：

[1] OSSERV ASTROFIS ARCETRI, FLORENCE, ITALY

来源：

关键词：

D O I：

10.1007/BF00152497

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

引用

页码：395 / 402

页数：8

共 16 条

[1] POLARIZATION INTERFEROMETER FOR 2800-MHZ SOLAR NOISE STUDIES WITH A 0.5' FAN BEAM
BELL, MB
COVINGTON, AE
KENNEDY, WAG
[J]. SOLAR PHYSICS, 1973, 28 (01) : 123 - 136
[2] STANFORD 5 ELEMENT RADIO TELESCOPE
BRACEWELL, RN
COLVIN, RS
DADDARIO, LR
GREBENKEMPER, CJ
PRICE, KM
THOMPSON, AR
[J]. PROCEEDINGS OF THE IEEE, 1973, 61 (09) : 1249 - 1257
[3] COVINGTON AE, 1973, UAG28 REP 1, P168
[4] FELLI M, 1974, ASTRON ASTROPHYS, V31, P431
[5] BRIGHTNESS DISTRIBUTION OF SUN AT 2.8 CM WAVELENGTH
FURST, E
HACHENBERG, O
ZINZ, W
HIRTH, W
[J]. SOLAR PHYSICS, 1973, 32 (02) : 445 - 458
[6] GIBSON EG, 1973, QUIET SUN, P31
[7] Grebenkemper C. J., 1973, Bulletin of the American Astronomical Society, V5
[8] HIGH-RESOLUTION RADIO OBSERVATIONS OF SUN AT 3.71 AND 11.1 CM
HOBBS, RW
JORDAN, SD
WEBSTER, WJ
[J]. NATURE-PHYSICAL SCIENCE, 1973, 243 (125): : 48 - 50
[9] SPECTROSCOPIC DETERMINATIONS OF SOLAR ROTATION
HOWARD, R
HARVEY, J
[J]. SOLAR PHYSICS, 1970, 12 (01) : 23 - &
[10] IKHSANOVA VN, 1960, P PULKOVO OBS, V21, P62