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Results: 1-16 |
Results: 16
Rates of flaring in individual active regions
Authors: Wheatland, MS
Citation: Ms. Wheatland, Rates of flaring in individual active regions, SOLAR PHYS, 203(1), 2001, pp. 87-106
Yohkoh/HXT evidence for a hyperhot loop-top source in the pre-impulsive phase of a loop flare
Authors: Uchida, Y Wheatland, MS Haga, R Yoshitake, I Melrose, D
Citation: Y. Uchida et al., Yohkoh/HXT evidence for a hyperhot loop-top source in the pre-impulsive phase of a loop flare, SOLAR PHYS, 202(1), 2001, pp. 117-130
Energy balance in the flaring solar corona
Authors: Wheatland, MS Litvinenko, YE
Citation: Ms. Wheatland et Ye. Litvinenko, Energy balance in the flaring solar corona, ASTROPHYS J, 557(1), 2001, pp. 332-336
Modeling the rate of occurrence of solar flares
Authors: Litvinenko, YE Wheatland, MS
Citation: Ye. Litvinenko et Ms. Wheatland, Modeling the rate of occurrence of solar flares, ASTROPHYS J, 550(1), 2001, pp. L109-L112
Metastable magnetic configurations and their significance for solar eruptive events
Authors: Sturrock, PA Weber, M Wheatland, MS Wolfson, R
Citation: Pa. Sturrock et al., Metastable magnetic configurations and their significance for solar eruptive events, ASTROPHYS J, 548(1), 2001, pp. 492-496
Do solar flares exhibit an interval-size relationship?
Authors: Wheatland, MS
Citation: Ms. Wheatland, Do solar flares exhibit an interval-size relationship?, SOLAR PHYS, 191(2), 2000, pp. 381-389
An optimization approach to reconstructing force-free fields
Authors: Wheatland, MS Sturrock, PA Roumeliotis, G
Citation: Ms. Wheatland et al., An optimization approach to reconstructing force-free fields, ASTROPHYS J, 540(2), 2000, pp. 1150-1155
The origin of the solar flare waiting-time distribution
Authors: Wheatland, MS
Citation: Ms. Wheatland, The origin of the solar flare waiting-time distribution, ASTROPHYS J, 536(2), 2000, pp. L109-L112
Flare frequency-size distributions for individual active regions
Authors: Wheatland, MS
Citation: Ms. Wheatland, Flare frequency-size distributions for individual active regions, ASTROPHYS J, 532(2), 2000, pp. 1209-1214
Are electric currents in solar active regions neutralized?
Authors: Wheatland, MS
Citation: Ms. Wheatland, Are electric currents in solar active regions neutralized?, ASTROPHYS J, 532(1), 2000, pp. 616-621
Frequency-energy distributions of flares and active region transient brightenings
Authors: Wheatland, MS Uchida, Y
Citation: Ms. Wheatland et Y. Uchida, Frequency-energy distributions of flares and active region transient brightenings, SOLAR PHYS, 189(1), 1999, pp. 163-172
Topological differences between force-free field models
Authors: Hudson, TS Wheatland, MS
Citation: Ts. Hudson et Ms. Wheatland, Topological differences between force-free field models, SOLAR PHYS, 186(1), 1999, pp. 301-310
Rotational signature and possible r-mode signature in the GALLEX solar neutrino data
Authors: Sturrock, PA Scargle, JD Walther, G Wheatland, MS
Citation: Pa. Sturrock et al., Rotational signature and possible r-mode signature in the GALLEX solar neutrino data, ASTROPHYS J, 523(2), 1999, pp. L177-L180
A better linear force-free field
Authors: Wheatland, MS
Citation: Ms. Wheatland, A better linear force-free field, ASTROPHYS J, 518(2), 1999, pp. 948-953
The waiting-time distribution of solar flare hard X-ray bursts
Authors: Wheatland, MS Sturrock, PA McTiernan, JM
Citation: Ms. Wheatland et al., The waiting-time distribution of solar flare hard X-ray bursts, ASTROPHYS J, 509(1), 1998, pp. 448-455
Apparent latitudinal modulation of the solar neutrino flux
Authors: Sturrock, PA Walther, G Wheatland, MS
Citation: Pa. Sturrock et al., Apparent latitudinal modulation of the solar neutrino flux, ASTROPHYS J, 507(2), 1998, pp. 978-983
Risultati: 1-16 |