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71.
Peter Kahabka 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2006,38(12):2836-2839
More than 100 supersoft X-ray sources (SSS) are reported in 20 external galaxies, the Magellanic Clouds (MCs) and our Galaxy. The effective temperatures of the brighter SSS are 20–100 eV. SSS with luminosities below ≈3 × 1038 erg s−1 are consistent with accreting white dwarfs (WDs) with steady nuclear burning or post-novae. Optical identifications exist for SSS in our Galaxy and the MCs (including orbital period determinations) and for SSS in M31 (with novae and symbiotic stars, SySs). High resolution X-ray spectra of the brightest SSS in our Galaxy and the MCs reveal the existence of spectral features due to high gravity WDs. Timing studies in X-rays (combined with the optical) of the stable nuclear burning phase in steady nuclear burning sources and in post-novae allow to constrain the mass accretion rate onto and the mass of the nuclear burning WD. The nature of a few SSS with luminosities 1039 erg s−1 remains unclear. 相似文献
72.
A. Belov 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2009
X-ray flares and acceleration processes are in one complex of sporadic solar events (together with CMEs, radio bursts, magnetic field dissipation and reconnection). This supposes the connection (if not physical, but at least statistical) between characteristics of the solar energetic proton events and flares. The statistical analysis indicates that probability and magnitude of the near-Earth proton enhancement depends heavily on the flare importance and their heliolongitude. These relations may be used for elaboration of the forecasting models, which allow us to calculate probability of the solar proton events from the X-ray observations. 相似文献
73.
O.S. Yakovchouk I.S. Veselovsky K. Mursula 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2009
We present and discuss here the first version of a data base of extreme solar and heliospheric events. The data base contains now 87 extreme events mostly since 1940. An event is classified as extreme if one of the three critical parameters passed a lower limit. The critical parameters were the X-ray flux (parameter R), solar proton flux (parameter S) and geomagnetic disturbance level (parameter G). We find that the five strongest extreme events based on four variables (X-rays SEP, Dst, Ap) are completely separate except for the October 2003 event which is one the five most extreme events according to SEP, Dst and Ap. This underlines the special character of the October 2003 event, making it unique within 35 years. We also find that the events based on R and G are rather separate, indicating that the location of even extreme flares on the solar disk is important for geomagnetic effects. We also find that S = 3 events are not extreme in the same sense as R > 3 and G > 3 events, while S = 5 events are missing so far. This suggests that it might be useful to rescale the classification of SEP fluxes. 相似文献
74.
R.K. Manchanda 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2011
We have developed a new detector using thin lanthanum bromide crystal (32 × 3 mm) for use in X-ray astronomy. The instrument was launched in high altitude balloon flight on two different occasions, December 21, 2007, which reached a ceiling altitude of 4.3 mbs and April 25, 2008 reaching a ceiling altitude 2.8 mbs. The observed background counting rate at the ceiling altitude of 4 mbs was ∼4 × 10−3 ct cm−2 s−1 keV−1 sr−1. This paper describes the details of the experiment, the detector characteristics, and the background behaviour at the ceiling altitude. 相似文献
75.
对于脉冲星试验01星的两年实测数据,针对蟹状星云脉冲星星历经历了多次更新的特点,提出了更新标准脉冲轮廓进行X射线计时的改进方法。以一系列观测时长为实测数据分组,再采用改进后的方法进行计时分析并与改进前的结果进行对比。通过对比改进前后的计时结果,发现改进方法得到的计时残差的均方根(root mean square, RMS)平均降低了14.2%,定位精度平均提高了14.4%,估计原子钟相对频率偏差的精度平均提高了26.2%,体现了改进方法处理经历多次星历更新的Crab脉冲星观测数据的合理性和优越性。此外,改进方法对脉冲星试验01星两年观测数据的稳定度σz没有量级上的改进,说明改进方法对Crab脉冲星时间稳定度的影响不大。 相似文献
76.
给出了1992-1995年Be/X射线双星LSI+61°303每年的光谱观测结果,分析了光谱发射线轮廓及其变化,观测显示Hβ发射线轮廓具有典型的气壳吸收,表明观测视线与Be星赤道平面平行,同时发现Hα发射线参数发等值宽度和双峰强度之比也具有类似射电流量的周期性变化,但其变化与射电玫光学光度的变化不同,因此认为此变化可能与中子星周期的吸积盘及其轨道交食有关。 相似文献
77.
78.
79.
G. Trottet 《Space Science Reviews》1994,68(1-4):149-158
Non-thermal hard X-ray, gamma-ray and radio emission are the most direct signatures of the presence of energetic particles in the solar atmosphere. This paper lays emphasis on hard X-ray and radio imaging data, obtained during and outside flares, which reveal the sites where particles interact with the ambient medium. These observations, which provide more or less direct information on the topology and dynamics of the magnetic structures in which particles are accelerated and propagate, are discussed in the framework of the statistical flare scenario. 相似文献
80.
R. Hudec Z. Ceplecha J. Ehrlich J. Borovi
ka K. Hurley J.-L. Ateia C. Barat M. Niel G. Vedrenne I.V. Estulin A.K. Kuznetsov V.M. Zenchenko T.L. Cline U. Desai W.D. Evans E. Fenimore R. Klebesadel J. Laros 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》1984,3(10-12)
The preliminary results from optical search for light pulses associated with gamma ray bursts by means of the Czechoslovak Fireball Network plate collection at the Ondřejov observatory are given. Optical monitoring represents more than 7700 hours, but no real optical counterpart was found. Problems associated with the optical search for gamma ray bursts are discussed. 相似文献