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Volumn 11, Issue 7, 2013, Pages 394-406

The 10.7 cm solar radio flux (F10.7)

Author keywords

10.7 cm Solar Radio Flux; F10.7; Penticton Flux

Indexed keywords


EID: 84881360022     PISSN: None     EISSN: 15427390     Source Type: Journal    
DOI: 10.1002/swe.20064     Document Type: Article
Times cited : (494)

References (22)
  • 1
    • 0043023089 scopus 로고
    • Microwave solar noise observations during the eclipse of November 23, 1946
    • Covington, A. E., (1947), Microwave solar noise observations during the eclipse of November 23, 1946, Nature, 159, 405-406.
    • (1947) Nature , vol.159 , pp. 405-406
    • Covington, A.E.1
  • 2
    • 0041520240 scopus 로고
    • Solar noise observations on 10.7 cm
    • Covington, A. E., (1948), Solar noise observations on 10.7 cm, Proc. IRE, 36, 454-457.
    • (1948) Proc. IRE , vol.36 , pp. 454-457
    • Covington, A.E.1
  • 4
    • 77955298548 scopus 로고    scopus 로고
    • Impact of changes in the Sun's conveyor belt on recent solar cycles
    • doi: 10.1029/2010GL044143.
    • Dikpati, M., P. A. Gilman, G. de Toma, and, R. K. Ulrich, (2010), Impact of changes in the Sun's conveyor belt on recent solar cycles, Geophys. Res. Lett., 37, doi: 10.1029/2010GL044143.
    • (2010) Geophys. Res. Lett. , vol.37
    • Dikpati, M.1    Gilman, P.A.2    De Toma, G.3    Ulrich, R.K.4
  • 5
    • 0001673220 scopus 로고
    • Large-scale patterns in solar activity during the ascending phase of cycle 21
    • Gaizauskas, V., K. L. Harvey, J. W. Harvey, and, C. Zwaan, (1983), Large-scale patterns in solar activity during the ascending phase of cycle 21, Astrophys. J., 65, 1056-1065.
    • (1983) Astrophys. J. , vol.65 , pp. 1056-1065
    • Gaizauskas, V.1    Harvey, K.L.2    Harvey, J.W.3    Zwaan, C.4
  • 7
    • 0003910623 scopus 로고
    • Introduction to solar radio astronomy and radio physics
    • 16, D. Reidel, Dordrecht, Netherlands.
    • Kruger, A., (1979), Introduction to solar radio astronomy and radio physics, Geophys. and Astrophys. Monogr., vol. 16, D. Reidel, Dordrecht, Netherlands.
    • (1979) Geophys. and Astrophys. Monogr
    • Kruger, A.1
  • 9
    • 0042021145 scopus 로고
    • Solar radiation at 1200 Mc/s, 600 Mc/s and 200 Mc/s
    • Lehaney, F. J., and, D. E. Yabsley, (1949), Solar radiation at 1200 Mc/s, 600 Mc/s and 200 Mc/s, Aust. J. Sci. Res. Ser. A, 2, 48-62.
    • (1949) Aust. J. Sci. Res. Ser. A , vol.2 , pp. 48-62
    • Lehaney, F.J.1    Yabsley, D.E.2
  • 10
    • 84866091373 scopus 로고    scopus 로고
    • Decreasing sunspot magnetic fields explain unique 10.7 cm radio flux
    • Livingston, W., M. J. Penn, and, L. Svalgaard, (2012), Decreasing sunspot magnetic fields explain unique 10.7 cm radio flux, Astrophys. J. Lett., 757, 8.
    • (2012) Astrophys. J. Lett. , vol.757 , pp. 8
    • Livingston, W.1    Penn, M.J.2    Svalgaard, L.3
  • 11
    • 33751092516 scopus 로고    scopus 로고
    • Temporal changes in-sunspot umbral magnetic fields and temperatures
    • DOI 10.1086/508345
    • Penn, M. J., and, W. Livingston, (2006), Temporal changes in sunspot umbral magnetic fields and temperatures, Astrophys. J., 649, L45-48. (Pubitemid 44770532)
    • (2006) Astrophysical Journal , vol.649 , Issue.II1
    • Penn, M.J.1    Livingston, W.2
  • 13
    • 0042020853 scopus 로고
    • Microwave proxies for sunspot blocking and total irradiance
    • Schmahl, E., and, M. R. Kundu, (1995), Microwave proxies for sunspot blocking and total irradiance, J. Geophys. Res., 100, 19,851-19,864.
    • (1995) J. Geophys. Res. , vol.100 , pp. 19
    • Schmahl, E.1    Kundu, M.R.2
  • 14
    • 0010129766 scopus 로고
    • Microwave radiation from the Sun
    • Southworth, G. C., (1945), Microwave radiation from the Sun, J. Franklin Inst., 239, 285-297.
    • (1945) J. Franklin Inst. , vol.239 , pp. 285-297
    • Southworth, G.C.1
  • 16
    • 79951807539 scopus 로고    scopus 로고
    • The solar microwave flux and sunspot number
    • in, edited by S. R. Cranmer, J. T. Hoeksema, and J. L. Kohl, Astronomical Society of the Pacific, San Francisco, Calif.
    • Svalgaard, L., and, H. S. Hudson, (2010), The solar microwave flux and sunspot number, in SOHO-23: Understanding a Peculiar Solar Minimum, ASP Conf. Ser., 428, edited by, S. R. Cranmer, J. T. Hoeksema, and, J. L. Kohl, pp. 325-328, Astronomical Society of the Pacific, San Francisco, Calif.
    • (2010) SOHO-23: Understanding A Peculiar Solar Minimum, ASP Conf. Ser., 428 , pp. 325-328
    • Svalgaard, L.1    Hudson, H.S.2
  • 17
    • 84881359408 scopus 로고
    • The absolute calibration of variable flux density in the microwave region
    • Tanaka, H., (1969), The absolute calibration of variable flux density in the microwave region, Prog. Radio Sci., 2, 1966-1969.
    • (1969) Prog. Radio Sci. , vol.2 , pp. 1966-1969
    • Tanaka, H.1
  • 19
    • 0000063899 scopus 로고
    • Recent solar radio astronomy at centimeter wavelengths: The variability of the 10.7 cm flux
    • Tapping, K. F., (1987), Recent solar radio astronomy at centimeter wavelengths: The variability of the 10.7 cm flux, J. Geophys. Res., 92, 829-838.
    • (1987) J. Geophys. Res. , vol.92 , pp. 829-838
    • Tapping, K.F.1
  • 20
    • 51249168846 scopus 로고
    • Limits to the accuracy of the 10.7 cm flux
    • Tapping, K. F., and, D. P. Charrois, (1994), Limits to the accuracy of the 10.7 cm flux, Sol. Phys., 150, 305-315.
    • (1994) Sol. Phys. , vol.150 , pp. 305-315
    • Tapping, K.F.1    Charrois, D.P.2
  • 21
    • 0011308310 scopus 로고
    • The origin of the 10.7 cm solar flux
    • Tapping, K. F., and, B. DeTracey, (1990), The origin of the 10.7 cm solar flux, Sol. Phys., 127, 321-332.
    • (1990) Sol. Phys. , vol.127 , pp. 321-332
    • Tapping, K.F.1    Detracey, B.2
  • 22
    • 80053910449 scopus 로고    scopus 로고
    • Did the Sun change its behaviour during the decline of cycle 23 and into cycle 24?
    • Tapping, K. F., and, J. J. Valdes, (2011), Did the Sun change its behaviour during the decline of cycle 23 and into cycle 24?, Sol. Phys., 272, 337-350.
    • (2011) Sol. Phys. , vol.272 , pp. 337-350
    • Tapping, K.F.1    Valdes, J.J.2


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.