nr |
titel |
auteur |
tijdschrift |
jaar |
jaarg. |
afl. |
pagina('s) |
type |
1 |
A fractal study on sunspot relative number
|
Zhang Qin, |
|
1994 |
18 |
3 |
p. 313-318 6 p. |
artikel |
2 |
A method for resolving the 180-degree ambiguity in the observed transverse field direction
|
Wang Jing-xiu, |
|
1994 |
18 |
3 |
p. 355- 1 p. |
artikel |
3 |
A new model of gamma-ray burst
|
Wei Da-ming, |
|
1994 |
18 |
3 |
p. 266-271 6 p. |
artikel |
4 |
An improved set of radiation hydrodynamic equations for stellar oscillation
|
Xiong Da-run, |
|
1994 |
18 |
3 |
p. 300-308 9 p. |
artikel |
5 |
An observed example of two sunspot groups colliding and merging LI
|
Bi-Qiang, |
|
1994 |
18 |
3 |
p. 352-353 2 p. |
artikel |
6 |
Application of symplectic algorithm to dynamical astronomy. III
|
Liu Lin, |
|
1994 |
18 |
3 |
p. 323-339 17 p. |
artikel |
7 |
A preliminary treatment of data from the full-disk magnetograph
|
Liu Yang, |
|
1994 |
18 |
3 |
p. 319-322 4 p. |
artikel |
8 |
A ring-like structure in the nuclear region of the post starburst galaxy NGC 4736
|
Gu Qiu-sheng, |
|
1994 |
18 |
3 |
p. 349-351 3 p. |
artikel |
9 |
A search for infrared objects in the Norma region
|
Xiao Zhen, |
|
1994 |
18 |
3 |
p. 282-288 7 p. |
artikel |
10 |
A simple physical analysis of the fine Hα structure in several active regions
|
Wu Bei, |
|
1994 |
18 |
3 |
p. 355-356 2 p. |
artikel |
11 |
A study of the e + e − → 3γ process in strong magnetic fields
|
Ping Jia-lun, |
|
1994 |
18 |
3 |
p. 241-247 7 p. |
artikel |
12 |
A two-component model for the infrared spectrum of AGB stars
|
Xiong Guan-Zhu, |
|
1994 |
18 |
3 |
p. 352- 1 p. |
artikel |
13 |
BD +47819: a peculiar flare star of spectral type A5
|
Wang Jun-jie, |
|
1994 |
18 |
3 |
p. 289-291 3 p. |
artikel |
14 |
Circumstellar OH maser observation of OH 17.7-2.0
|
Yu Zhi-yao, |
|
1994 |
18 |
3 |
p. 309-312 4 p. |
artikel |
15 |
COS-B identification of the new γ pulsar PSR 1055-52
|
Song Li-ming, |
|
1994 |
18 |
3 |
p. 272-274 3 p. |
artikel |
16 |
Effect of horizontal motion of photospheric matter on filament activation and solar flare
|
Yin Chun-Lin, |
|
1994 |
18 |
3 |
p. 352- 1 p. |
artikel |
17 |
Intermittent chaos in pulsating stars
|
Chen Fu-sheng, |
|
1994 |
18 |
3 |
p. 292-299 8 p. |
artikel |
18 |
KS entropy of measure-preserving mappings with parabolic fixed point
|
Zhou Ji-lin, |
|
1994 |
18 |
3 |
p. 340-348 9 p. |
artikel |
19 |
Methods of precise determination of light energy concentration of telescopes
|
Su Ding-qiang, |
|
1994 |
18 |
3 |
p. 353-354 2 p. |
artikel |
20 |
Modulation imaging γ-ray telescope
|
Li Ti-pei, |
|
1994 |
18 |
3 |
p. 275-278 4 p. |
artikel |
21 |
Monte Carlo simulation of quasar spectrum and selection effects in multicolor survey of high-redshift quasars
|
Fan Xiao-Hui, |
|
1994 |
18 |
3 |
p. 354- 1 p. |
artikel |
22 |
On the loss of angular momentum in cataclysmic binaries
|
Bi Shao-Lan, |
|
1994 |
18 |
3 |
p. 354-355 2 p. |
artikel |
23 |
Recommended sets of integration coefficients for solving differential equations of the form y″ = F(X,Y)
|
Xu Ji-hong, |
|
1994 |
18 |
3 |
p. 353- 1 p. |
artikel |
24 |
The annual variation in the groud-based astronomical observational residuals caused by anomalous refraction
|
Gao Bu-xi, |
|
1994 |
18 |
3 |
p. 353- 1 p. |
artikel |
25 |
The environment of galaxy formation and the cosmic voids
|
Ma Er, |
|
1994 |
18 |
3 |
p. 248-256 9 p. |
artikel |
26 |
The possibility of overtaking between the components of a superluminal source
|
Hong Xiao-Yu, |
|
1994 |
18 |
3 |
p. 354- 1 p. |
artikel |
27 |
The propagation of chromospheric condensation and the asymmetry of spectral lines of solar flares
|
Ding Ming-De, |
|
1994 |
18 |
3 |
p. 355- 1 p. |
artikel |
28 |
The stable regions of triangular libration points of the planets. II
|
Zhao Chang-Yin, |
|
1994 |
18 |
3 |
p. 353- 1 p. |
artikel |
29 |
Two-point correlation function, correlation fractal dimension and typical scales in the large-scale distribution of IRAS galaxies
|
Liu Bin, |
|
1994 |
18 |
3 |
p. 257-265 9 p. |
artikel |
30 |
X-ray pulsations in the radio pulsar PSR 1951 +32
|
Cheng Ling-xiang, |
|
1994 |
18 |
3 |
p. 279-281 3 p. |
artikel |