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131.
Dana Procházková Vít Kárník Ivan Brouček Reviewer A. Zátopek 《Studia Geophysica et Geodaetica》1980,24(1):102-103
an¶rt;u am mu 15- an 1979. a auu a mumuu auu. 相似文献
132.
Lubomír Kubáček Lea Bartalošová Ján Pecár Reviewer F. Charamza 《Studia Geophysica et Geodaetica》1977,21(3-4):227-235
Summary If the condition R(A)=k(n), whereA is the design matrix of the type n × k and k the number of parameters to be determined, is not satisfied, or if the covariance matrixH is singular, it is possible to determine the adjusted value of the unbiased estimable function of the parameters f(), its dispersion D(
(x)) and
2
as the unbiased estimate of the value of
2
by means of an arbitrary g-inversion of the matrix
. The matrix
, because of its remarkable properties, is called the Pandora Box matrix. The paper gives the proofs of these properties and the manner in which they can be employed in the calculus of observations. 相似文献
133.
Václav Bucha Reviewer F. Rein Reviewer J. Bochníček 《Studia Geophysica et Geodaetica》1977,21(3-4):350-360
Summary As a result of investigating the relations between the variations of geomagnetic activity and meteorological factors [1, 2] a mechanism of solar-terrestrial relationships and a model of the changes of atmospheric circulation in the Northern Hemisphere are proposed; this provides an explanation of the causes of the fluctuation of the climate, of dry and cold periods and differing vegetation conditions in various years in dependence on the intensity of geomagnetic activity. 相似文献
134.
135.
Summary As a result of investigating the energy flow, transmitted by short-period HM waves, the existence of a frequency limitation was found at the theoretical investigation of the propagation of these HM waves. 相似文献
136.
137.
František Rein 《Studia Geophysica et Geodaetica》1972,16(3):306-306
Ohne Zusammenfassung 相似文献
138.
Ümit Kiziloğlu Altan Baykal Murat Alev Ersin Göğüş 《Astrophysics and Space Science》1998,259(2):191-203
Using archival ASCA and ROSAT observations of RE 0751+14, X- ray energy spectra, pulse profiles and the results of pulse timing
analysis are presented. The energy spectra are well-fitted by a blackbody model at low energy and a Raymond-Smith model at
high energy, together with a partial covering absorber. A fluorescence emission line at 6.4 keV with an equivalent width ∼
220 eV was resolved for the first time.
This revised version was published online in July 2006 with corrections to the Cover Date. 相似文献
139.
M. Ćwiok W. Dominik K. Małek L. Mankiewicz J. Mrowca-Ciułacz K. Nawrocki L. W. Piotrowski P. Sitek M. Sokołowski G. Wrochna A. F. Żarnecki 《Astrophysics and Space Science》2007,309(1-4):531-535
Experiment “Pi of the Sky” is designed to search for prompt optical emission from GRB sources. 32 CCD cameras covering 2 steradians will monitor the sky continuously. The data will be analysed on-line in search for optical flashes. The prototype with 2 cameras operated at Las Campanas (Chile) since 2004 has recognised several outbursts of flaring stars and has given limits for a few GRB. 相似文献
140.
Martin Nekola René Hudec Martin Jelínek Matůš Kocka Petr Kubánek Filip Münz Cyril Polášek Vojtěch Šimon Jan Štrobl 《Experimental Astronomy》2010,28(1):79-85
We report on two small aperture robotic telescopes called BART and D50 operated in Ondřejov. Both telescopes are capable of
automatic observation of gamma ray burst (GRB) optical afterglows. Coordinates of GRBs are taken from alerts distributed via
Internet. Telescopes observe other interesting high energy sources when there is not any alert. The smaller telescope BART
has aperture D = 254 mm. The bigger telescope D50 has a primary mirror of diameter D = 500 mm. Both telescopes are controlled
by free software package RTS2 and are accessible through Internet. We describe the two telescopes and related software and
show some results such as our first observed optical counterpart of GRB. 相似文献