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Title:   Kandilli Rasathanesi'nde 1949 Ocak ayından 1951 Haziran ayına kadar yapılan Güneş leke resatları.
Authors:   Dizer, Muammer
Journal:   Istanbul, Milli Egitim Basimevi, 1953.
Publication Date:   00/1953
Origin:   LOC
LOC Keywords:   SUN-SPOTS
Comment:   LCCN: ne62-40(PREM); CALL NUMBER: QB525 .D56 (Orien Turk)
Bibliographic Code:   1953QB525.D56......

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Title:   Les observations des taches solaires faites a l'Observatoire de Kandilli DU 12 janvier 1949 AU 30 juin 1951.
Authors:   Dizer, Muammer
Journal:   Istanbul, Milli Egitim Basimevi, 1953.
Publication Date:   00/1953
Origin:   LOC
LOC Keywords:   SUN-SPOTS
Comment:   LCCN: 61-46363(PREM); CALL NUMBER: QB525 .D58
Bibliographic Code:   1953QB525.D58......

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Title:   Sur le cycle de 80 ans de l'activité solaire
Authors:   Dizer, Muammer
Journal:   Annales d'Astrophysique, Vol. 19, p.207
Publication Date:   01/1956
Origin:   ADS
Bibliographic Code:   1956AnAp...19..207D

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Title:   Long-lived filaments and geomagnetic storms
Authors:   Dizer, M.
Journal:   The Observatory, Vol. 82, p. 250-253 (1962)
Publication Date:   12/1962
Origin:   OBS
Bibliographic Code:   1962Obs....82..250D

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Title:   Kandilli Observatory, Istanbul
Authors:   Dizer, M.
Journal:   Solar Physics, Vol. 3, p.491 (SoPh Homepage)
Publication Date:   00/1968
Origin:   ADS
Bibliographic Code:   1968SoPh....3..491D

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Title:   A Typical Twisted Surge on November 10, 1967
Authors:   Dizer, M.
Journal:   Solar Physics, Vol. 4, p.99 (SoPh Homepage)
Publication Date:   00/1968
Origin:   ADS
Bibliographic Code:   1968SoPh....4...99D

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Title:   Isophotal Photometry and Morphological Changes in the Flares
Authors:   Dizer, M.
Journal:   Solar Physics, Vol. 10, p.416 (SoPh Homepage)
Publication Date:   00/1969
Origin:   ADS
Bibliographic Code:   1969SoPh...10..416D

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Title:   Isophotometric Measurements of Mercury
Authors:   Dizer, M.; Yazici, M. N.
Journal:   Astrophysics and Space Science, Vol. 13, p.106 (Ap&SS Homepage)
Publication Date:   00/1971
Origin:   ADS
Bibliographic Code:   1971Ap&SS..13..106D

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Title:   A loop prominence system observed on May 24, 1972
Authors:   Dizer, M.
Affiliation:   AA(Kandilli Observatory, Istanbul, Turkey)
Journal:   Solar Physics, vol. 59, Oct. 1978, p. 357-360. (SoPh Homepage)
Publication Date:   10/1978
Category:   Solar Physics
Origin:   STI
NASA/STI Keywords:   H ALPHA LINE, SOLAR FLARES, SOLAR PROMINENCES, SOLAR X-RAYS, SUNSPOTS, K LINES, SOLAR SPECTRA, X RAY SPECTRA
Bibliographic Code:   1978SoPh...59..357D

Abstract

A flare-loop prominence appeared over a complex sunspot group in McMath region No. 11895, on May 24, 1972. The evolution of the loop prominence and its relation to a flare were observed using H-alpha and Ca K filters. Soft X-ray emission between 0.5-20 A was found to be emitted from the flare-loop prominence system.

 

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Title:   International Symposium on the Observatories in Islam - Sep19-23,1977, 1980
Authors:   Dizer, Muammer
Journal:   International Symposium on the Observatories in Islam, September 19-23, 1977. Editor, Muammer Dizer; Publisher, Milli Egitim Basimevi, Istanbul, 1980. ISBN # NONE. LC # QB82.I8 I57 1977.
Publication Date:   00/1980
Origin:   ADS
Bibliographic Code:   1980isot.symp.....D

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Title:   Book-Review - on the Observatories in Islam - International Symposium 1977SEP19-23
Authors:   Dizer, M.; Kennedy, E. S.
Journal:   JOURNAL FOR THE HISTORY OF ASTRONOMY V. 13, P. 64, 1982
Publication Date:   00/1982
Origin:   KNUDSEN
Bibliographic Code:   1982JHA....13...64D

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Title:   A calculation method for the visibility curve of the new moon
Authors:   Dizer, Muammer
Journal:   [Istanbul] : Bosphorus University : Kandilli Observatory, [1984?]
Publication Date:   00/1984
Origin:   LOC
LOC Keywords:   NEW MOON: VISIBILITY: MEASUREMENT
Comment:   LCCN: 84-202758(BKS3); CALL NUMBER: QB588 .D59 1984
Bibliographic Code:   1984QB588.D59......

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Title:   Astronomi Hazineleri
Authors:   Dizer, Muammer
Journal:   [Istanbul] : Bogazici Universitesi, Kandilli Rasathanesi, 1986. 1. baski.
Publication Date:   00/1986
Origin:   LOC
LOC Keywords:   KANDILLI RASATHANESI, ASTRONOMICAL INSTRUMENTS: TURKEY: HISTORY, ASTRONOMICAL OBSERVATORIES: TURKEY: ISTANBUL
Comment:   LCCN: 87-968477(BKS3); CALL NUMBER: QB85 .D59 1986 
Bibliographic Code:   1986QB85.D59.......

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Title:   Rubu Tahtası
Authors:   Dizer, Muammer
Journal:   Istanbul : Bogazici Universitesi, 1987.
Publication Date:   00/1987
Origin:   LOC
LOC Keywords:   QUADRANT
Comment:   LCCN: 87-968781(BKS3); CALL NUMBER: QB105 .D59 1987 
Bibliographic Code:   1987QB105.D59......

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Title:   Spectral studies of the time-series of the geomagnetic activities
Authors:   Dizer, M.; Ozguc, A.
Affiliation:   AB(Kandilli Observatory, Istanbul, Turkey)
Journal:   Earth, Moon, and Planets (ISSN 0167-9295), vol. 43, Dec. 1988, p. 211-220. (EM&P Homepage)
Publication Date:   12/1988
Category:   Geophysics
Origin:   STI
NASA/STI Keywords:   GEOMAGNETISM, MAGNETIC EFFECTS, SPECTRUM ANALYSIS, TIME SERIES ANALYSIS, ANNUAL VARIATIONS, FOURIER TRANSFORMATION, POWER SPECTRA
Bibliographic Code:   1988EM&P...43..211D

Abstract

The geomagnetic effects of solar active centers and the seasonal variation of geomagnetic activity are examined. The periodicities of aa, Ci, and Ap indices are studied using discrete Fourier transforms. It is found that recurrent storm days do not significantly increase when the frequency of sporadic storm days increases as the active centers approach the sun-earth line.

 

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Title:   Periodicity and distribution of the sudden disappearances of solar prominences in the chromosphere
Authors:   Dizer, Muammer
Affiliation:   AA(Kandilli Observatory, Istanbul, Turkey)
Journal:   Astrophysics and Space Science (ISSN 0004-640X), vol. 173, no. 1, Nov. 1990, p. 127-144. (Ap&SS Homepage)
Publication Date:   11/1990
Category:   Solar Physics
Origin:   STI
NASA/STI Keywords:   CHROMOSPHERE, SOLAR PROMINENCES, POWER SPECTRA, SOLAR ATMOSPHERE, SYMMETRY
Bibliographic Code:   1990Ap&SS.173..127D

Abstract

The periodicity and the distribution of the sudden disappearance (SD) of the solar prominences on the chromosphere are studied. The spectral analysis of the SD, from 1039 to 1762 Carrington rotation number, shows a typical period at 138 (10.3 yr) solar rotations in the northern hemisphere and at 153 (11.4 yr) solar rotations in the southern hemisphere of the sun. The power-spectral analysis of the asymmetry index yields a primary peak at 155 (11.6 yr) solar rotations. By plotting the distribution of SD along the Carrington longitude, it can be seen that the distribution of the SD is nearly uniform.

 

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Title:   Periodicity in filamentary activity
Authors:   Dizer, Muammer
Affiliation:   AA(Kandilli Observatory, Istanbul, Turkey)
Journal:   Astrophysics and Space Science (ISSN 0004-640X), vol. 189, no. 2, March 1992, p. 289-301. (Ap&SS Homepage)
Publication Date:   03/1992
Category:   Solar Physics
Origin:   STI
NASA/STI Keywords:   PERIODIC VARIATIONS, SOLAR PROMINENCES, POWER SPECTRA, SOLAR ATMOSPHERE, SPECTRUM ANALYSIS
Bibliographic Code:   1992Ap&SS.189..289D

Abstract

This paper presents the results of the study on the periodicity in filament activity. The spectral analysis of the number of filaments shows a basic period at 141 (10.5 yr), at 138 (10.3 yr), and at 144 (10.7 yr) Carrington rotation in the Northern and Southern Hemisphere, respectively. The time series concerning the index of filament activity also shows a typical period at 135 Carrington rotation (about 10.1 yr) at 144 Carrington rotation (about 10.7 yr) and at 133 Carrington rotation (about 9.9 yr), respectively, in the Northern and Southern Hemisphere. The power spectrum analysis of the time series of the filamentary activity in the short-term also yields less pronounced but still noticeable peaks which are statistically significant.

 

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Title:   The relation between electric conductivity in faculae and in the Bilderberg model of the photosphere
Authors:   Kopeck?, M.; Soytürk, E.
Journal:   Bulletin of the Astronomical Institute of Czechoslovakia, vol. 22, p.154
Publication Date:   00/1971
Origin:   ADS
Bibliographic Code:   1971BAICz..22..154K

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Title:   North-south asymmetries in the green corona brightness between 1947 and 1976
Authors:   Ozguc, Atila; Ucer, Cumhure
Affiliation:   AB(Kandilli Observatory, Istanbul, Turkey)
Journal:   Solar Physics (ISSN 0038-0938), vol. 114, no. 1, 1987, p. 141-146. (SoPh Homepage)
Publication Date:   00/1987
Category:   Solar Physics
Origin:   STI
NASA/STI Keywords:   ASYMMETRY, BRIGHTNESS, PERIODIC VARIATIONS, POWER SPECTRA, SOLAR CORONA, SOLAR SPECTRA, PHOTOSPHERE, SOLAR ACTIVITY, SOLAR CYCLES, SUNSPOTS
Bibliographic Code:   1987SoPh..114..141O

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Title:   Kinematics of a twisted surge
Authors:   Ozguc, Atila; Duzgelen, Ayten
Affiliation:   AB(Kandilli Observatory, Istanbul, Turkey)
Journal:   Astrophysics and Space Science (ISSN 0004-640X), vol. 150, no. 2, Dec. 1988, p. 383-386. (Ap&SS Homepage)
Publication Date:   12/1988
Category:   Solar Physics
Origin:   STI
NASA/STI Keywords:   H ALPHA LINE, MAGNETOHYDRODYNAMICS, SOLAR PROMINENCES, SOLAR MAGNETIC FIELD, SOLAR RADIATION, TWISTING
Bibliographic Code:   1988Ap&SS.150..383O

Abstract

Using the H-alpha solar filtergrams taken at Kandilli Observatory, the motion of a twisted surge has been studied from the kinematic point of view. The Palus (1972) method has been applied to two knots of the twisted surge occurred at November 10, 1967. The results are discussed.

 

 
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Title:   Spectral studies of the time-series of the geomagnetic activities
Authors:   Dizer, M.; Ozguc, A.
Affiliation:   AB(Kandilli Observatory, Istanbul, Turkey)
Journal:   Earth, Moon, and Planets (ISSN 0167-9295), vol. 43, Dec. 1988, p. 211-220. (EM&P Homepage)
Publication Date:   12/1988
Category:   Geophysics
Origin:   STI
NASA/STI Keywords:   GEOMAGNETISM, MAGNETIC EFFECTS, SPECTRUM ANALYSIS, TIME SERIES ANALYSIS, ANNUAL VARIATIONS, FOURIER TRANSFORMATION, POWER SPECTRA
Bibliographic Code:   1988EM&P...43..211D

Abstract

The geomagnetic effects of solar active centers and the seasonal variation of geomagnetic activity are examined. The periodicities of aa, Ci, and Ap indices are studied using discrete Fourier transforms. It is found that recurrent storm days do not significantly increase when the frequency of sporadic storm days increases as the active centers approach the sun-earth line.

 

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Title:   Solar rotation rate from stable sunspot tracings
Authors:   Ozguc, Atila; Saglamsaatci, Mualla
Affiliation:   AB(Kandilli Observatory, Istanbul, Turkey)
Journal:   Astrophysics and Space Science (ISSN 0004-640X), vol. 153, no. 2, March 1989, p. 345-349. (Ap&SS Homepage)
Publication Date:   03/1989
Category:   Solar Physics
Origin:   STI
NASA/STI Keywords:   ANGULAR VELOCITY, SOLAR ROTATION, SUNSPOTS, LEAST SQUARES METHOD, LONG TERM EFFECTS, NORTHERN HEMISPHERE, POSITION (LOCATION), SOUTHERN HEMISPHERE
Bibliographic Code:   1989Ap&SS.153..345O

Abstract

Positions of sunspots between 1966 and 1976 as observed at Kandilli Observatory were used to determine the differential rotation of the sun. A total of 202 sunspot groups which were E, F, G, H, and J-types were chosen, and a least-squares solution was calculated with their daily rotations. A gradient difference was found between the two hemispheres of the sun.

 

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Title:   Distribution of LDE flares on the sun during solar cycles 20 and 21
Authors:   Ozguc, Atila; Duzgelen, Ayten
Affiliation:   AB(Kandilli Observatory, Cengelkoy, Turkey)
Journal:   Astrophysics and Space Science (ISSN 0004-640X), vol. 162, no. 1, Dec. 1989, p. 27-33. (Ap&SS Homepage)
Publication Date:   12/1989
Category:   Solar Physics
Origin:   STI
NASA/STI Keywords:   SOLAR CYCLES, SOLAR FLARES, PROBABILITY DISTRIBUTION FUNCTIONS, SOLAR X-RAYS
Bibliographic Code:   1989Ap&SS.162...27O

Abstract

The latitude and longitude (northern and southern hemispheric) distributions based on 2277 LDE flares observed during the period from 1966 to 1986 have been studied. It is found that there exist active zones, in which the LDE flare occurrence rate is much higher. Latitudinal belts between 11-20 deg and longitudinal belts around 80-100 deg are the most prolific places to produce LDE flares. During cycles 20 and 21 these active zones produced 36 percent of the total number of LDE flares by occupying only 6 percent area of the sun.

 

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Title:   78-day periodicity in the solar 1-8 A X-ray index during the ascending branch of cycle 21
Authors:   Ozguc, Atila
Affiliation:   AA(Kandilli Observatory, Cengelkoy, Turkey)
Journal:   Astrophysics and Space Science (ISSN 0004-640X), vol. 162, no. 1, Dec. 1989, p. 123-127. (Ap&SS Homepage)
Publication Date:   12/1989
Category:   Solar Physics
Origin:   STI
NASA/STI Keywords:   SOLAR ACTIVITY, SOLAR CYCLES, SOLAR X-RAYS, FOURIER TRANSFORMATION, POWER SPECTRA
Bibliographic Code:   1989Ap&SS.162..123O

Abstract

The time series of 1-8 A X-ray index for the time interval between January 1977 to September 1981 has been analyzed by calculating the power spectrum using the discrete Fourier transform. A 78-day periodicity, which is one-half of the period found from various solar parameters of cycles 20 and 21 by various authors, was found. This periodicity is thought to be related to the 152-day periodicity.

 

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Title:   Periodic behavior of solar flare index during solar cycles 20 and 21
Authors:   Ozguc, Atila; Atac, Tamer
Affiliation:   AB(Kandilli Observatory, Istanbul, Turkey)
Journal:   Solar Physics (ISSN 0038-0938), vol. 123, no. 2, 1989, p. 357-365. (SoPh Homepage)
Publication Date:   00/1989
Category:   Solar Physics
Origin:   STI
NASA/STI Keywords:   PERIODIC VARIATIONS, SOLAR CYCLES, SOLAR FLARES, FACULAE, SOLAR ACTIVITY, SUNSPOT CYCLE
Bibliographic Code:   1989SoPh..123..357O

Abstract

Short-term periodicities of solar activity were studied with the flare index by using Discrete Fourier Transform for the time interval 1966-1986. Two noticeable periodicities (18.5 and 5 months) have been found. The existence of these periodicities comparing with the early findings is discussed.

 

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Title:   On the Latitudinal Distribution of the Solar Surges
Authors:   Ozguc, A.
Journal:   SOLAR PHYSICS V.123, NO. 2, P.381, 1989 (SoPh Homepage)
Publication Date:   00/1989
Origin:   KNUDSEN
Bibliographic Code:   1989SoPh..123..381O

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Title:   Distribution of solar surges
Authors:   Ozguc, A.; Yesilyaprak, H.; Duzgelen, A.
Affiliation:   AC(Kandilli Observatory, Istanbul, Turkey)
Journal:   Astronomy and Astrophysics (ISSN 0004-6361), vol. 241, no. 1, Jan. 1991, p. 209-211. (A&A Homepage)
Publication Date:   01/1991
Category:   Solar Physics
Origin:   STI
NASA/STI Keywords:   SOLAR ACTIVITY EFFECTS, SOLAR FLARES, SOLAR TERRESTRIAL INTERACTIONS, ANNUAL VARIATIONS, MAGNETIC DISTURBANCES, SUNSPOTS, SURGES
Bibliographic Code:   1991A&A...241..209O

Abstract

Latitudinal and longitudinal (northern and southern hemispheric) distributions were studies, based on 1456 flare-related solar surges observed during the period from 1980 to 1988. It is found that there exist some active longitude belts where the surge production is more profuse in each hemisphere of the sun. Latitudinal belts between + or - 11 deg and + or - 20 deg and longitudinal belts around 0 - 10 deg and 270 - 280 deg are the most prolific zones to produce surges. During the period 1980-1988 those active zones produced 22 percent of the total number of surges while occupying less than 10 percent of the solar surface. There is good correlation with earlier findings of active longitudes.

 

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Title:   Intermediate-term periodicities in the green corona brightness of the sun
Authors:   Ozguc, Atila
Affiliation:   AA(Kandilli Observatory, Istanbul, Turkey)
Journal:   Astrophysics and Space Science (ISSN 0004-640X), vol. 187, no. 2, Jan. 1992, p. 197-207. (Ap&SS Homepage)
Publication Date:   01/1992
Category:   Solar Physics
Origin:   STI
NASA/STI Keywords:   EMISSION SPECTRA, IRRADIANCE, PERIODIC VARIATIONS, SOLAR CORONA, SOLAR SPECTRA, FOURIER TRANSFORMATION, SOLAR ACTIVITY, SOLAR CYCLES
Bibliographic Code:   1992Ap&SS.187..197O

Abstract

Intermediate-term periodicities in the green corona were analyzed by dividing 10-deg latitudinal belts for the solar cycles 18, 19, and 20 (1947-1976). Discrete Fourier transform technique was used and three noticeable periodicities (3.48, 2.57, and 2.27 yr) were found. The period of 3.48-yr period is the strongest one, and the 17.6-m periodicity was found only around the +40-deg belt while 155-d periodicity was not revealed.

 

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Title:   The 73-day periodicity of the flare index during the current solar cycle 22
Authors:   Ozguc, Atila; Atac, Tamer
Affiliation:   AABogazici University, Istanbul, Turkey ABBogazici University, Istanbul, Turkey
Journal:   Solar Physics, vol. 150, no. 1-2, p. 339-346 (SoPh Homepage)
Publication Date:   03/1994
Category:   Solar Physics
Origin:   STI
NASA/STI Keywords:   GAMMA RAY ASTRONOMY, GAMMA RAY BURSTS, LIGHT (VISIBLE RADIATION), PERIODIC VARIATIONS, PHOTOSPHERE, SOLAR ACTIVITY, SOLAR CORONA, SOLAR CYCLES, SOLAR FLARES, SOLAR PROTONS, SOLAR X-RAYS, SUNSPOTS, X RAY ASTRONOMY, BRIGHTNESS, CORRELATION, FALSE ALARMS, FOURIER ANALYSIS, FOURIER TRANSFORMATION, POWER SPECTRA, PROBABILITY THEORY, RANDOM NOISE, SPECTRUM ANALYSIS, TIME SERIES ANALYSIS
Bibliographic Code:   1994SoPh..150..339O

Abstract

The flare index of the current solar cycle 22 is analysed to detect periodicities. Power spectral analysis of the time series of solar flare index data reveals a periodicity around 73 and 53 days. We find that a periodicity of 73 days was in operation from November 1988 to the end of December 1991. We also find that when the 73-day periodicity or the 154-day periodicity is in operation the flare index is well correlated with the relative sunspot numbers.

 

 
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Title:   The 73-DAY Periodicity of the Flare Index during the Current SOLAR-CYCLE-22
Authors:   Ozguc, A.; Atac, T.
Journal:   SOLAR PHYSICS V.152, NO. 1/JUN, P.318, 1994 (SoPh Homepage)
Publication Date:   06/1994
Origin:   KNUDSEN
Bibliographic Code:   1994SoPh..152..318O

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Title:   Confirmation of the 25.5-Day Fundamental Period of the Sun Using the North-South Asymmetry of the Flare Index
Authors:   Ozguc, Atila; Atac, Tamer
Journal:   Solar Physics, v. 163, p. 183-191. (SoPh Homepage)
Publication Date:   01/1996
Origin:   KLUWER
Bibliographic Code:   1996SoPh..163..183O

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Title:   Longitudinal Distribution of Flares in the Late Phase of Active Regions
Authors:   Ozguc, Atila; Altas, Levent
Journal:   Solar Physics, v. 163, p. 327-333. (SoPh Homepage)
Publication Date:   02/1996
Origin:   KLUWER
Bibliographic Code:   1996SoPh..163..327O

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Title:   North-South Asymmetry in the Solar Flare Index
Authors:   Atac, Tamer; Ozguc, Atila
Journal:   Solar Physics, v. 166, p.201 (SoPh Homepage)
Publication Date:   06/1996
Origin:   ADS
Bibliographic Code:   1996SoPh..166..201A

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Title:   Examination of the solar cycle variation of foF2 by using solar flare index for the cycle 21
Authors:   Özgüç, A.; Tulunay, Y.; Ataç, T.
Affiliation:   AA(Kandilli Observatory, Bog˘azi çi University, Çengelköy Istanbul, Turkey), AB(Middle East Technical University, Dept. of Aeronautical Eng. 06531 Ankara, Turkey), AC(Kandilli Observatory, Bog˘aziçi University, Çengelköy Istanbul, Turkey)
Journal:   Advances in Space Research, Volume 22, Issue 1, p. 139-142. (AdSpR Homepage)
Publication Date:   00/1998
Origin:   ELSEVIER
Abstract Copyright:   (c) 1998 Elsevier Science B.V. All rights reserved.
Bibliographic Code:   1998AdSpR..22..139O

Abstract

For solar cycle 21 (1976 - 1986) the variation of monthly mean values of noon-time foF2 at Slough, Rome, and Manila are examined by using solar flare index and geomagnetic Ap index. A single regression analysis for dependence of foF2 on solar flare index shows better matching. Moreover, less hysteresis effect is seen when we use solar flare index instead of other solar indices. Thus, for making prediction, one needs to take into account just the solar flare index and not the solar flare index and geomagnetic Ap index simultaneously.

 

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Title:   Flare Index of Solar Cycle 22
Authors:   Atac, Tamer; Ozguc, Atila
Journal:   Solar Physics, v. 180, Issue 1/2, p. 397-407. (SoPh Homepage)
Publication Date:   06/1998
Origin:   KLUWER
Bibliographic Code:   1998SoPh..180..397A

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Title:   The last total solar eclipse of the millennium in Turkey
Authors:   Ozguc, A.; Atac, T.; Altas, L.
Journal:   Contributions of the Astronomical Observatory Skalnate Pleso, vol. 28, no. 3, p. 285-289. (CoSka Homepage)
Publication Date:   03/1999
Origin:   COSKA
Keywords:   THE SUN, SOLAR ECLIPSE
Bibliographic Code:   1999CoSka..28..285O

Abstract

The last total solar eclipse of the millennium will be observed from Turkey which bridges two continents and has been the cradle of so many past civilizations. Wouldn't you like to witness this magnificent event in the mystic ambiance of central Anatolia which offers its guests Turkish hospitality and a lot of historical examples of paganism, Christianity and Islam. Among the countries from which the eclipse will be visible, Turkey seems to be one of the most suitable countries in terms of its climate and observational facilities. Kandilli Observatory and Earthquake Research Institute has arranged fieldwork on the eclipse path to determine the suitable points for the observations. The shadow of the moon will be first seen from the Black Sea coast at 14:20 L.T. It will then pass through central Anatolia and will leave Turkey from south-east at 14:42 L.T.

 

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Title:   The Last Total Eclipse of the Millennium
Authors:   Livingston, W.; Özgüc, A.
Journal:   The Publications of the Astronomical Society of the Pacific, Volume 111, Issue 766, pp. 1597-1597. (PASP Homepage)
Publication Date:   12/1999
Origin:   UCP
PASP Keywords:   CONFERENCE HIGHLIGHTS
Abstract Copyright:   (c) 1999: The Astronomical Society of the Pacific
Bibliographic Code:   1999PASP..111.1597L

Abstract

Conference was held in Istanbul, Turkey, in 1999 August. Proceedings will be edited by W. Livingston and A. Özgüc and published in the ASP Conference Series.

 

 
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Title:   Preparations for the Last Total Solar Eclipse of the Millenium in Turkey
Authors: