quick-relievers
发表于 2025-3-21 19:49:31
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affluent
发表于 2025-3-21 21:26:12
Fei Xu,Fangming Liu,Dekang Zhu,Hai Jin and 3rd stages of the vehicle, a transfer orbit with a low apogee (12 000 km instead of the required 36 000 km) was reached. This deficiency was such that the satellite’s onboard apogee boost motor could not turn this anomalous transfer orbit into anything near a geostationary orbit. The motor was,
jovial
发表于 2025-3-22 03:25:54
Tao Jiang,Xiaowei Xu,Lu Pu,Yu Hu,Zhijun Qiuhe performance of the experiment is outlined to demonstrate that electric fields can be measured with accuracies of ±0.7 mV m . and ± 1.0 mV m. in the dawn-dusk and satellite-sun directions respectively. These uncertainties can be considerably reduced under favourable plasma conditions. Examples of
arabesque
发表于 2025-3-22 08:13:54
Fei Xu,Fangming Liu,Dekang Zhu,Hai Jinnt categories of emissions: waves with frequencies below the proton gyrofrequency .. and frequencies above. Belonging to the first category are the structured ULF events called ‘pearls’ which are very often observed on the ground, but which were observed only twice on board GEOS-1 in seven months of
Interregnum
发表于 2025-3-22 12:48:30
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overwrought
发表于 2025-3-22 13:01:45
Ying Wang,Dongfeng Wang,Fengyin Li a theoretical linear instability model of an electrostatic cyclotron harmonic wave event recorded on GEOS-1. The presence of a hot loss cone component of the particle distribution is established experimentally, and the model accounts reasonably for the observed frequencies and relative strengths of
借喻
发表于 2025-3-22 17:37:15
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乳汁
发表于 2025-3-22 23:26:47
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affluent
发表于 2025-3-23 01:39:01
Linkun Zhang,Yuxia Lei,Zhengyan Wang mode and the corresponding telemetry data were recorded at the NASA stations. For two passes over Jim Creek (48°2’N– 121°9’W) where a powerful VLF transmitter (.. = 18.6 kHz) is located, GEOS was put in a specific mode in order to study the magnetospheric electromagnetic field in the vicinity of ..
Dislocation
发表于 2025-3-23 06:32:57
Linkun Zhang,Yuxia Lei,Zhengyan Wangons in amplitude and in . ratio on a time scale of 0.1 s. The time delay of the signals vary considerably over a period of a few minutes, and often the duration of the received pulses on the dipole antenna is longer than the duration of the transmitted pulses. The propagation aspects of these observ