Helium fluxes measured by the PAMELA experiment from the minimum to the maximum solar activity for solar cycle 24

被引：0

作者：

University of Rome Tor Vergata, Department of Physics, Rome ^{[1
]}

I-00133, Italy

不详 ^{[2
]}

I-00133, Italy

不详 ^{[3
]}

I-34149, Italy

不详 ^{[4
]}

I-34014, Italy

不详 ^{[5
]}

I-34100, Italy

不详 ^{[6
]}

D-57068, Germany

不详 ^{[7
]}

2520, South Africa

不详 ^{[8
]}

24118, Germany

不详 ^{[9
]}

I-50019, Italy

不详 ^{[10
]}

I-50019, Italy

不详 ^{[11
]}

I-80126, Italy

不详 ^{[12
]}

I-80126, Italy

不详 ^{[13
]}

RU-119991, Russia

不详 ^{[14
]}

I-70126, Italy

不详 ^{[15
]}

I-70126, Italy

不详 ^{[16
]}

RU-194021, Russia

不详 ^{[17
]}

MD, United States

不详 ^{[18
]}

DC, United States

不详 ^{[19
]}

SE-10691, Sweden

不详 ^{[20
]}

不详 ^{[21
]}

I-50019, Italy

不详 ^{[22
]}

RU-115409, Russia

不详 ^{[23
]}

90570, Finland

不详 ^{[24
]}

I-00044, Italy

不详 ^{[25
]}

00133, Italy

不详 ^{[26
]}

机构：

来源：

arXiv |

关键词：

D O I：

暂无

中图分类号：

学科分类号：

摘要：

Cosmology - Helium - Solar energy - Solar radiation - Solar wind - Spectroscopy

引用

共 50 条

[31] Monitoring solar activity during 23/24 solar cycle minimum through VLF radio signals
Kolarski, A.
Sreckovic, V. A.
Mijic, Z. R.
CONTRIBUTIONS OF THE ASTRONOMICAL OBSERVATORY SKALNATE PLESO, 2022, 52 (03): : 105 - 115
[32] Solar- diurnal variations of cosmic rays from the maximum to the minimum of solar activity
DORMAN LI
KOLOMEYETS YEV
1600,
[33] Variations in Oscillation Frequencies From Minimum to Maximum of Solar Activity
Kiran Jain
A. Bhatnagar
Solar Physics, 2003, 213 : 257 - 268
[34] Variations in oscillation frequencies from minimum to maximum of solar activity
Jain, K
Bhatnagar, A
SOLAR PHYSICS, 2003, 213 (02) : 257 - 268
[35] Heliospheric Effect on Solar Activity Parameters during Maximum Phase of Solar Cycle 24(2012–2015)
PRSingh
Upendra KrSingh Kushwaha
AKSingh
TKPant
Research in Astronomy and Astrophysics, 2024, 24 (12) : 3 - 12
[36] Solar activity: Towards a standard classification of solar phases from cycle 1 to cycle 24
Sawadogo, Saguedo
Gnabahou, Doua Allain
Pahima, Tinle
Ouattara, Frederic
ADVANCES IN SPACE RESEARCH, 2024, 73 (01) : 1041 - 1049
[37] Evidence for distinctive changes in the solar wind helium abundance in solar cycle 24
Yogesh
Chakrabarty, D.
Srivastava, N.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2021, 503 (01) : L17 - L22
[38] Solar origins of solar wind properties during the cycle 23 solar minimum and rising phase of cycle 24
Luhmann, Janet G.
Petrie, Gordon
Riley, Pete
JOURNAL OF ADVANCED RESEARCH, 2013, 4 (03) : 221 - 228
[39] Interplanetary Scintillations of the Radio Source Ensemble at the Maximum of Cycle 24 of Solar Activity
Chashei, I. V.
Shishov, V. I.
Tyul'bashev, S. A.
Subaev, I. A.
COSMIC RESEARCH, 2016, 54 (03) : 178 - 184
[40] Interplanetary scintillations of the radio source ensemble at the maximum of cycle 24 of solar activity
I. V. Chashei
V. I. Shishov
S. A. Tyul’bashev
I. A. Subaev
Cosmic Research, 2016, 54 : 178 - 184

← 1 2 3 4 5 →