✦ LIBER ✦

Facular excess radiation and the energy balance of solar active regions

✍ Scribed by M. Steinegger; H. Haupt; P. N. Brandt; W. Schmidt

Publisher: Springer
Year: 1994
Tongue: English
Weight: 35 KB
Volume: 152
Category: Article
ISSN: 0038-0938
DOI: 10.1007/bf01473225

No coin nor oath required. For personal study only.

📜 SIMILAR VOLUMES

The gross energy balance of solar active

The gross energy balance of solar active regions

✍ Kenton D. Evans; J. P. Pye; R. J. Hutcheon; M. Gerassimenko; A. S. Krieger; J. M 📂 Article 📅 1977 🏛 Springer 🌐 English ⚖ 331 KB

According to Parker's earlier articles in this journal the photospheric temperature is lower in sunspots than elsewhere because of increased outflow of mechanical energy, rather than inhibited inflow from the convective zone. In this case the atmosphere above the spot group receives an excess supply

Energy balance in solar active regions:

Energy balance in solar active regions: The dip of April, 1985

✍ H.S. Hudson 📂 Article 📅 1986 🏛 Elsevier Science 🌐 English ⚖ 190 KB

The correlation of solar flare productio

The correlation of solar flare production with magnetic energy in active regions

✍ E. B. Mayfield; John K. Lawrence 📂 Article 📅 1985 🏛 Springer 🌐 English ⚖ 677 KB

An investigation of 531 active regions was made to determine the correlation between energy released by flares and the available energy in magnetic fields of the regions. Regions with magnetic flux greater than 102~ maxwell during the years 1967-1969, which included sunspot maximum, were selected fo

Comments on the heating of solar active

Comments on the heating of solar active regions by magnetic energy dissipation

✍ Suresh Chandra 📂 Article 📅 1986 🏛 Springer Netherlands 🌐 English ⚖ 81 KB

Cyclotron lines in the spectra of solar

Cyclotron lines in the spectra of solar flares and solar active regions

✍ V. V. Zheleznyakov; E. Ya. Zlotnik 📂 Article 📅 1989 🏛 Springer 🌐 English ⚖ 387 KB

It was shown by Zheleznyakov and Zlotnik (1980a, b) that in complex configurations of solar magnetic fields (in hot loops above the active centres, in neutral current sheets in the preflare phase, in hot X-ray kernels in the initial flare phase) a system of cyclotron lines in the spectrum of microwa

Plasma radiation diagnostics of the prim

Plasma radiation diagnostics of the primary energy release region in solar flares

✍ Dean F. Smith; Daniel S. Spicer 📂 Article 📅 1979 🏛 Springer 🌐 English ⚖ 854 KB

The possibility is investigated that the plasma turbulence used in many recent models of the primary energy release and acceleration in solar flares should be detectable by radiation near the fundamental and second harmonic of the plasma frequency. Formulae are derived for fundamental emission due t