1.EVOLUTION OF VECTOR MAGNETIC-FIELDS AND VERTICAL CURRENTS AND THEIR RELATIONSHIP WITH SOLAR-FLARES IN AR-5747

WANG, TJ, XU, AA, ZH     More...

WANG, TJ, XU, AA, ZHANG, HQ     Less

SOLAR PHYSICS[0038-0938], Published 1994, Volume 155, Issue 1, Pages 99-112

收錄情况： WOS SCOPUS

WOS核心合集引用: 80  2024影響因子:  2.4 

2.STABILITY OF THE LUNDQUIST FIELD AND THE PHYSICAL NATURE OF ERUPTIVE PROMINENCES WITH HELICAL STRUCTURE

XU, AA, WU, GP     More...

XU, AA, WU, GP     Less

SOLAR PHYSICS[0038-0938], Published 1995, Volume 159, Issue 2, Pages 265-273

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WOS核心合集引用: 5  2024影響因子:  2.4 

3.Filament current systems and solar flares

Tang, YH, Cui, LS, Y     More...

Tang, YH, Cui, LS, Yin, CL, Xu, AA     Less

SOLAR PHYSICS[0038-0938], Published 1996, Volume 168, Issue 2, Pages 297-309

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WOS核心合集引用: 0  2024影響因子:  2.4 

4.The observational evidence on the loop-loop interaction in a flare-CME event on April 15, 1998

Wu, GP, Huang, GL, T     More...

Wu, GP, Huang, GL, Tang, YH, Xu, AA     Less

SOLAR PHYSICS[0038-0938], Published 2005, Volume 227, Issue 2, Pages 327-337

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WOS核心合集引用: 3  2024影響因子:  2.4  发表年影響因子:  1.892 

5.The Calibrations for the Chang'E-2 Solar X-Ray Monitor

Dong, WD, Zhang, XP,     More...

Dong, WD, Zhang, XP, Li, Y, Tang, CL, Xu, AA, Zhang, F     Less

SOLAR PHYSICS[0038-0938], Published 2019, Volume 294, Issue 9,

收錄情况： WOS SCOPUS

WOS核心合集引用: 5  2024影響因子:  2.4  发表年影響因子:  2.503