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Co-Authors
- Moni Chaudhary
- M. C. Ramadevi
- S. Seetha
- Dipankar Bhattacharya
- B. T. Ravishankar
- N. Sitaramamurthy
- G. Meena
- M. Ramakrishna Sharma
- Ravi Kulkarni
- V. Chandra Babu
- Brajpal Singh
- Anand Jain
- Reena Yadav
- S. Vaishali
- B. N. Ashoka
- Anil Agarwal
- K. Balaji
- Manoj Kumar
- Prashanth Kulshresta
- Pankaj Agarwal
- Mathew Sebastian
- K. Sankarasubramanian
- Manju Sudhakar
- Anuj Nandi
- Abhijit Avinash Adoni
- Ankur Kushwaha
- Arjun Dey
- Bhuwan Joshi
- V. Girish
- Ishan Tomar
- Kamal Kumar Majhi
- Manjunath Olekar
- Monoj Bug
- Manohar Pala
- Mukund Kumar Thakur
- Rajeev R. Badagandi
- Sarthak Garg
- N. Sridhara
- C. N. Umapathy
- Vinod Kumar Gupta
- Vivek Kumar Agrawal
- B. Yougandar
- V. Radhakrishna
- A. Tyagi
- S. Narendranath
- Koushal Vadodariya
- G. Balaji
- Neeraj Satya
- Akash Shetty
- H. N. Suresha Kumar
- Netra S. Pillai
- S. Tadepalli
- Venkata Raghavendra
- P. Sreekumar
- N. Valarmathi
A B C D E F G H I J K L M N O P Q R S T U V W X Y Z All
Kumar,
- The effectiveness of reiki and accupressure on insomnia and depression
Abstract Views :1078 |
Authors
Moni Chaudhary
1,
Kumar
2
Affiliations
1 Department of Psychology, Meerut College, Meerut, UP, IN
2 Department of Psychology, Chaudhary Charan singh University, Meerut, IN
1 Department of Psychology, Meerut College, Meerut, UP, IN
2 Department of Psychology, Chaudhary Charan singh University, Meerut, IN
Source
Indian Journal of Positive Psychology, Vol 3, No 4 (2012), Pagination: 411-414Abstract
The aim of the present study was to investigate the combined effect of reiki and acupressure on insomnia and depression in female sufferers. The sample was consisted of 40 female subjects of age group 30-45 years with high scores on symptoms of insomnia and depression. Subjects were randomly selected on the basis of scores of self-developed 'Insomnia Scale' and 'Amritsar Depression Inventory'. The selected subjects were randomly assigned to two groups of experimental (20 Ss) and control group (20 Ss) having more or less equal variance of insomnia and depression scores. The reiki healing and acupressure was applied twice a week for 10 weeks on experimental group. Data was collected before and after the treatment from both groups. Obtained data were analyzed through mean and ANCOVA. The results show that the reiki and acupressure together were significantly effective methods in reducing insomnia and depression symptoms in female sufferers.
- Scanning Sky Monitor On-Board AstroSat
Abstract Views :258 |
PDF Views:90
Authors
M. C. Ramadevi
1,
S. Seetha
2,
Dipankar Bhattacharya
3,
B. T. Ravishankar
1,
N. Sitaramamurthy
1,
G. Meena
1,
M. Ramakrishna Sharma
1,
Ravi Kulkarni
1,
V. Chandra Babu
1,
Kumar
1,
Brajpal Singh
1,
Anand Jain
1,
Reena Yadav
1,
S. Vaishali
1,
B. N. Ashoka
1,
Anil Agarwal
1,
K. Balaji
4,
Manoj Kumar
5,
Prashanth Kulshresta
5,
Pankaj Agarwal
6,
Mathew Sebastian
6
Affiliations
1 Space Astronomy Group, SSIF, ISITE Campus, Karthik Nagar, Outer Ring Road, ISRO Satellite Centre, Bengaluru 560 037, IN
2 Indian Space Research Organisation Headquarters, Department of Space, Antariksh Bhavan, New BEL Road, Bengaluru 560 231, IN
3 Inter-University Centre for Astronomy and Astrophysics, Post Bag 4, Ganeshkhind, Pune 411 007, IN
4 Spacecraft Mechanisms Group, ISAC, Old Airport Road, Vimanapura Post, Bengaluru 560 017, IN
5 Control and Digital Electronics Group, ISAC, Old Airport Road, Vimanapura Post, Bengaluru 560 017, IN
6 Vikram Sarabhai Space Center, Thiruvananthapuram 695 022, IN
1 Space Astronomy Group, SSIF, ISITE Campus, Karthik Nagar, Outer Ring Road, ISRO Satellite Centre, Bengaluru 560 037, IN
2 Indian Space Research Organisation Headquarters, Department of Space, Antariksh Bhavan, New BEL Road, Bengaluru 560 231, IN
3 Inter-University Centre for Astronomy and Astrophysics, Post Bag 4, Ganeshkhind, Pune 411 007, IN
4 Spacecraft Mechanisms Group, ISAC, Old Airport Road, Vimanapura Post, Bengaluru 560 017, IN
5 Control and Digital Electronics Group, ISAC, Old Airport Road, Vimanapura Post, Bengaluru 560 017, IN
6 Vikram Sarabhai Space Center, Thiruvananthapuram 695 022, IN
Source
Current Science, Vol 113, No 04 (2017), Pagination: 599-601Abstract
Scanning Sky Monitor (SSM) on-board AstroSat is a wide-field imager to monitor the X-ray sky in the energy band 2.5-10 keV. The primary science objective of SSM is to detect and locate transient X-ray sources in the sky. Once detected the information is to be provided to the astronomical community for follow-up observations to do a more detailed study of the source. Long-term monitoring of known X-ray transient sources is also one of the science objectives of SSM. The instrument constitutes three units of 1D positionsensitive propotional counters with coded masks on each, all three mounted on a platform capable of rotation to scan about 50% of the sky in one full rotation. The angular resolution of each unit in SSM is 12' x 2.5°. Sensitivity of SSM is ~30 milliCrab at 3 sigma in 10 min integration time. This article briefly discusses the instrument and a few early results since the launch of AstroSat.Keywords
AstroSat, Crab, Scanning Sky Monitor, X-Ray Transient Sources.Full Text
References
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- X-Ray Spectrometers On-Board Aditya-L1 for Solar Flare Studies
Abstract Views :212 |
PDF Views:66
Authors
K. Sankarasubramanian
1,
Manju Sudhakar
1,
Anuj Nandi
1,
M. C. Ramadevi
1,
Abhijit Avinash Adoni
1,
Ankur Kushwaha
1,
Anil Agarwal
1,
Arjun Dey
1,
Bhuwan Joshi
2,
Brajpal Singh
1,
V. Girish
1,
Ishan Tomar
1,
Kamal Kumar Majhi
1,
Kumar
1,
Manjunath Olekar
1,
Monoj Bug
1,
Manohar Pala
1,
Mukund Kumar Thakur
1,
Rajeev R. Badagandi
1,
B. T. Ravishankar
1,
Sarthak Garg
1,
N. Sitaramamurthy
1,
N. Sridhara
1,
C. N. Umapathy
1,
Vinod Kumar Gupta
1,
Vivek Kumar Agrawal
1,
B. Yougandar
1
Affiliations
1 ISITE Campus, ISRO Satellite Centre, Outer Ring Road, Marathahalli, Bengaluru 560 037, IN
2 Udaipur Solar Observatory, Physical Research Laboratory, Udaipur 313 004, IN
1 ISITE Campus, ISRO Satellite Centre, Outer Ring Road, Marathahalli, Bengaluru 560 037, IN
2 Udaipur Solar Observatory, Physical Research Laboratory, Udaipur 313 004, IN
Source
Current Science, Vol 113, No 04 (2017), Pagination: 625-627Abstract
Aditya-L1 mission will carry two high-spectral resolution X-ray spectrometers to study solar flares. The soft X-ray spectrometer will cover the energy range from 1 to 30 keV, while the hard X-ray spectrometer will cover from 10 to 150 keV. These two instruments together will provide opportunities to study the plasma parameters during solar flares as well as acceleration mechanisms of energetic particles during the flaring time.Keywords
Coronal Heating, Solar Flares, X-Ray Spectrometers.Full Text
References
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- Hannah, I. G. et al., Microflares and the statistics of X-ray flares. Space Sci. Rev., 2011, 159, 263–300.
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- Joshi, B. et al., Pre-flare activity and magnetic reconnection during the evolutionary stages of energy release in a solar eruptive flare. ApJ, 2011, 743, 195–208.
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- Yashiro, S. et al., Spatial relationship between solar flares and coronal mass ejections. ApJ, 2008, 673, 1174–1180.
- Chifor, C. et al., The early phases of a solar prominence eruption and associated flare: a multi-wavelength analysis. A&A, 2006, 458, 965–973.
- Warmuth, A. et al., Rapid changes of electron acceleration characteristics at the end of the impulsive phase of an X-class solar flare. ApJ, 2009, 699, 917.
- SoLEXS Team, SoLEXS PDR document, ISRO-ISACADITYA-L1RR-1343, 2016.
- HEL1OS Team, HEL1OS PDR document, ISRO-ISAC-ADITYA-L1RR-1342, 2016.
- Chandrayaan-2 Large Area Soft X-ray Spectrometer
Abstract Views :269 |
PDF Views:85
Authors
V. Radhakrishna
1,
A. Tyagi
1,
S. Narendranath
1,
Koushal Vadodariya
1,
Reena Yadav
1,
Brajpal Singh
1,
G. Balaji
1,
Neeraj Satya
1,
Akash Shetty
1,
H. N. Suresha Kumar
1,
Kumar
1,
S. Vaishali
1,
Netra S. Pillai
1,
S. Tadepalli
1,
Venkata Raghavendra
1,
P. Sreekumar
2,
Anil Agarwal
1,
N. Valarmathi
1
Affiliations
1 U.R. Rao Satellite Centre, ISRO, Bengaluru 560 017, IN
2 Space Science Programme Office, ISRO Head Quarters, Bengaluru 560 017, IN
1 U.R. Rao Satellite Centre, ISRO, Bengaluru 560 017, IN
2 Space Science Programme Office, ISRO Head Quarters, Bengaluru 560 017, IN
Source
Current Science, Vol 118, No 2 (2020), Pagination: 219-225Abstract
Chandrayaan-2 Large Area Soft X-ray Spectrometer (CLASS) is an X-ray fluorescence spectrometer experiment aimed at mapping the abundances of major rock-forming elements on the lunar surface. The instrument consists of swept charge devices with a passive collimator, visible light blocking filters and signal processing electronics designed and built at U.R. Rao Satellite Centre, Indian Space Research Organisation. CLASS will be the largest collecting area spectrometer flown to the Moon, and thus is expected to map the abundances of lunar elements with a higher sensitivity than ever at soft X-ray energies.Keywords
Moon, Rock-forming Elements, Spectrometer, X-ray Fluorescence.Full Text
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