Editor-in-Chief : V.K. Rastogi
|AJP||ISSN : 0971 – 3093
Vol 16, No. 1, January-March, 2007
Vol. 16, No 1 (2007) 1-9
Variation in area and intensity of the solar chromospheric network elements and their contribution to UV irradiance variability
R Kariyappa, B A Varghese and L Dame*
Indian Institute ofAstrophysics, Bangalore 560 034, India
*Service d’Aeronomie du CNRS, BP # 3, 91371 Verrieres-le-Buisson Cedex, France
The Sun is the primary source of energy responsible for governing both the weather and climate of Earth. For that reason alone one would expect that changes in the amount and type of energy Earth received from the Sun could alter weather and climate on the Earth. The variations in the UV irradiance are produced by surface manifestation of solar magnetic activity. Considering the variations in the solar UV flux may cause significant changes in the Earth’s climate, understanding the physical origin of UV irradiance changes is an extremely important issue in Solar and Space Physics.
We have segregated the (i) plages, (ii) magnetic network, and (iii) intranetwork + the background regions from the CaII K spectroheliograms of 1980 and 1992, observed at the National Solar Observatory at Sacramento Peak, using their histograms taken for the full-disk. The different parameters like the intensity and area of the chromospheric features, the full-disk intensity (spatial K index), and the full width at half maximum (FWHM) of the histograms , have been derived from the images. The spatial K index, FWHM, and the intensity of various features have been compared to the UV irradiance measured in the MgII h and k lines by the Nimbus7 and NOAA9 satellites and it has been found that they are correlated with the MgII h and k c/w ratio. We established, for the first time, from the results of 1992 images  and of 1980 that the FWHM can be used as a good index for measuring and describing the chromospheric activity in the K-line. The results of both 1980 and 1992 images show an anticorrelation between the intensity and area of the network elements, which confirm the earlier findings derived entirely from different data set from Kodaikanal CaII K spectroheliograms analyzed for the center of the solar disc in a quiet regions for a longer time interval of 1957 to 1983 . During solar minimum the network is fainter but covers a larger area than during solar maximum. These results suggest that the variations in both the intensity and area of the various chromospheric features have to be taken into account in irradiance models.
Keywords: Chromospheric features, Spatial K index, full width at half maximum (FWHM)
© Anita Publications. All rights reserved.
Total Refs: 24
1. Kariyappa R, Pap J M, Solar Phys,167(1996)115.
2. Kariyappa R, Sivaraman K R, Solar Phys, 152(1994)139.
3. Foukal P, Lean L, Astrophys J, 328(1988)347.
4. Lean J L, J Geophys Res, 91(1987)5567.
5. Barth C A, Tobiska W K, Rottman G J, White O R, J Geophys Res Lett, 17(1990)571.
6. Livingston W C, in Elizabeth Nesme-Ribes (ed), The Solar Engine and its Influence on Terrestrial Atmosphere and Climate, NATO ASI Series, 1993, p 145.
7. Pap J, Astron Astrophys, 264(1992)249.
8. Sofia S L, Oster L, Schatten K H, Solar Phys, 80(1982)87.
9. Lean J L, White O R, Livingston W C,Heath D F, Donnelly R F, Skumanich A, J Geophys Res,87(1982)10307.
10. Worden J R, White O R, Woods T N, Astrophys J, 496(1998)998.
11. Kariyappa R, J Astrophys Astron, 21(2000)2293.
12. Skumanich A, Smythe C, Frazier E N, Astrophys J, 200(1975)747.
13. Sivaraman K R, Livingston W C, Solar Phys,80(1982)227.
14. Nindos A, Zirin H, Solar Phys, 179(1998)253.
15. Sivaraman K R,,Gupta S S, Livingston W C, Dame L, Kalkofen W, Keller C U, Smartt R, Hasan S S, Astron Astrophys, 363(2000)279.
16. Harvey K L, White O R, Astrophys J, 515(1999)812.
17. White O R, Livingston W C, Astrophys J, 249(1981)798.
18. Sivaraman K R, Singh J, Bagare S P, Gupta S S, Astrophys J,313(1987)456.
19. Lean J L,J Geophys Res, 92(1987)839.
20. Muller R, Roudier Th, Solar Phys,152(1994)131.
21. Ermolli I, Berrilli F, Florio A, Pietropaolo E, in K S Balasubramaniam, J W Harvey,Rabin D M (eds), Synoptic Solar Physics, ASP Conference series Vol 140, 1998,p 223.
22. Berrilli F, Florio A, Ermolli I, Solar Phys,180(1998)29.
23. Berrilli F, Ermolli I, Florio A, Pietropaolo E, Astron astrophys,344(1999)965.
Vol 16, No 1 (2007) 11-16
The study of Raman, FT-IR reflection and transmission spectroscopy of acidic α-LiIO3 crystal and its birefringence properties
R Malekfar and M Rezvani Jalal
Faculty of Basic Sciences, Tarbiat Modarres University, P.O. Box 14115-175, Tehran, I. R. Iran
α-LiIO3 crystal has found wide spread applications in second harmonic generation, nonlinear optics, one dimensional ionic conductors and acousto-optic modulators especially in the visible and near infrared region. This crystal was grown from acidic saturated solution of α-LiIO3 salt by the method of slow evaporation of isothermal solution with about 1 × 1 2 cm3 dimensions. In the visible region this crystal is transparent and is a negative uniaxial crystal. The Raman, FT-IR reflection and transmission spectra of this crystal from both surfaces parallel and perpendicular to the crystal optical axis were obtained. With the help of Kramers – Kronig relations of reflection the ordinary and extra- ordinary refractive indices in the 400 – 4000 cm-1 region were calculated and it was shown that in this range, and particularly in the 700 -900 cm-1 region, this crystal converts to a positive uniaxial crystal. The imaginary part of the refractive index and the electrical susceptibilities of the crystal in the mentioned directions and in the 400 – 1000 cm-1 region were also calculated.
Keywords: LiIO3 crystal, Raman and FT-IR reflection, Kramers – Kronig relations
©Anita Publications. All rights reserved.
Total Refs: 10
1. Gaffar M A, Abu El-Fadl A, Journal of Physics and Chemistry of Solids, 60(1999)1633.
2. Pimenta M A, J Phys Condens Matter, 9(1997)7903.
3. Pask H M, Progress in Quantum Electronics, 27(2003)3.
4. Mugnier Y, Galez C, Solid State Communications,115(2000)619.
5. Righi A, Oliveria M A S, Solid State Ionics, 148(2002)203.
6. Mugnier Y, Galez C, J Solid State Chem ,168(2002)76.
7. Chen W C, Li C R, J Crystal Growth, 254(2003)162.
8. Galez C, Mugnier Y, Optical Materials, 19(2002)33.
9. Robertson D S,Roslington J M, J Phys D:Appl Phys, 4(1971)1582.
Vol 16, No 1 (2007) 23-27
Synthesis and spectral studies of Co(II), Ni(II) and Cu(II) complexes with Schiff bases derived from 2-methyl-thioquinazolin-4(3H) one*
B K Rai1, Irena Kostova2, S P Ojha3, Rashmi Tomar4 and V K Rastogi4
1Department of Chemistry, LNT College, (BRA Bihar University), Muzaffarpur-842 002, India
of Chemistry, Faculty of Pharmacy, Medical University, 2 Dunav St, Sofia-1000,
3Vice Chancellor, CCS University, Meerut-205 004, India
Mixed ligand Schiff base complexes of the type [M(MTSC)2X2] and [M(MTTSC)2X2], where M = Co(II), Ni(II) and Cu(II), MTSC = 2-methyl-thioqionazolin-4(3H) one semicarbazone, MTTSC = 2-methyl-thioquinazolin-4(3H) one thiosemicarbazone and X = Cl–, Br – and I– have been isolated. The ligands and complexes have been characterised by elemental analysis, infrared and electronic spectra, magnetic susceptibility and conductivity data. On the basis of I.R. spectra, the ligands, MTSC and MTTSC have been proposed to act in a bidentate manner, co-ordinating to the metal ions through the azomethine nitrogen and oxygen/sulphur atoms of either semicarbazone or thiosemicarbazone moiety. The remaining co-ordination sites are occupied by anions such as Cl–, Br– and Electronic spectral and magnetic susceptibility data proposed octahedral geometry of the complexes around the central metal ion. The complexes were found to be non-electrolytic in nature. © Anita Publications. All rights reserved.
1. Naranshima Murty, T S Dharrnaranjan, Asian J Chem, 14 (2002) 1325.
2. Thomas Joby, Parameswaram Geetha, Asian J Chem, 14 (2002) 1354.
3. Taylor M R, Glusker J P, Grabe E J, Minkin J A, Bioinorg Chem, 3 (1974) 89.
4. Padye S. Kauffaman G B, Coord Chem Rev, 63 (1985) 127.
5. Albertini, Bonati A, Lunghi P, Pieeli S, J Inorg Biochem, 70 (1998) 145.
6. Rai B K, Baluni Akhilesh, Asian J Chem, 14 (2002) 305.
7. Rai B K, Choudhry Pramod, Asian J Chem, 14 (2002) 305.
8. Rai B K, Sharma K, Singh A K, Asian J Chem, 14 (2002) 1556.
9. Rai B K. Sharma K, Asian J Phys, 11 (2002) 103.
10. Rai B K, Asian J Chem, 14 (2002) 1589.
11. Rai B K, Rai H C, Baluni D C, Prasad P R, Kumar A, Orient J Chem, 18 (2002) 575.
12. Rai B K, Kumar Mukesh, J Indian Council Chem, 20 (2003) 22.
13. Rai B K, Rai R, Orient J Chem, 20 (2004) 493; 601.
14. Rai B K, Kumar K, Shreevastava Y P, Asian J Chem, 17 (2005) 1773.
15. Das G C, Mahapatra B K, J Indian Chem Soc, 61 (1984) 831.
16. Vogel A I, A textbook of quantitative chemical analysis, revised by Bessett J. Denny R C. Jeffery G H and Mendham J, 5th edn. (1996).
17. Patil M S, Shah J R, J Indian Chem Soc, 58 (1981) 944.
18. Chaterjee B, Coord Chem Revs, 26 (9978) 281.
19. Rao N R, Rao P V, Reddy G V, Ganorkar M C, Indian J Chem, 26A (1987) 887.
20. Goldstien M, Unsworth D.Inorg Chim Acta, 4 (1970) 342.
21. Chaube S N, Shreevastava J P. Mishra L K, Inorg Chim Acta, 23 (1977) 1.
22. Gadag R G Gajendragad M R, Indian J Chem, 16A (1978) 703.
23. Singh N K, Shrivastava A K, Agarwal R C. Indian J Chem, 22A (1984) 704.
24. Nakamoto K. Infrared Spectra of inorganic and co-ordiantion compounds, (John Wiley & Sons, New York).
Vol 16, No 1 (2007)80-82
On the nature of scattering of some tea samples of Assam
N Dehingia, R Changrnai and G D Baruah
Department of Physics, Dibrugarh University, Dibrugarh – 786 004, India
Scattered radiation at wavelength 6328Å from nine samples of blended tea solutions of different qualities have been investigated. Intensity measurements of the radiations indicate a possible correlation with the quality of the sample. © Anita Publications. All rights reserved
1. Rayleight Lord, Scientific Paper ( Cambridge University Press. Cambridge). Vol. 1 and 4, ( 1912).
2. Chenery E M. Trace Elements in Tea, 6 (1955) 174.
3. Bandhu H K, Singh B, Chand B , Garg M L, Singh Nrimal, Baruah G D, Mangal P C, Proc Nat Sym Rad Phv 11( 1995) 244.