Detection of sources of periodic radio emission with the Large Phased Array of the Lebedev Physical Institute

2017 ◽  
Vol 61 (1) ◽  
pp. 30-37 ◽  
Author(s):  
A. E. Rodin ◽  
V. V. Oreshko ◽  
V. A. Samodurov
Keyword(s):  
Radio Emission ◽  
Phased Array ◽  
Lebedev Physical Institute ◽  
Physical Institute ◽  
Lebedev Physical

Observations of Corotating Streams of the Solar Wind with the Large Phased Array of the Lebedev Physical Institute in 2016

2019 ◽  
Vol 63 (5) ◽  
pp. 409-419 ◽  
Author(s):  
I. V. Chashei ◽  
S. A. Tyul’bashev ◽  
I. A. Subaev ◽  
A. I. Chernyshova
Keyword(s):  
Solar Wind ◽  
Phased Array ◽  
Lebedev Physical Institute ◽  
Physical Institute ◽  
Lebedev Physical

Observations of the gamma-ray pulsar J1836+5925 at 111 MHz

2021 ◽  
Vol 30 (1) ◽  
pp. 119-121
Author(s):  
Maria Timirkeeva ◽  
Igor Malov ◽  
Valery Malofeev ◽  
Oleg Malov
Keyword(s):  
Phased Array ◽  
Gamma Ray ◽  
Lebedev Physical Institute ◽  
Astronomical Observatory ◽  
Radio Observations ◽  
Physical Institute ◽  
Lebedev Physical

Abstract We describe the 10-day radio observations of the gamma-ray pulsar J1836+5925. Observations were carried out in the Pushchino Radio Astronomical Observatory at the frequency of 111 MHz using the Large Phased Array of the Lebedev Physical Institute.

scholarly journals Old Supernova Remnants: Structure and Source of Radio Emission

1987 ◽  
Vol 40 (6) ◽  
pp. 713 ◽  
Author(s):  
AP Glushak ◽  
AV Kovalenko ◽  
SM Kutuzov ◽  
AV Pynzar' ◽  
VA Udal’tsov
Keyword(s):  
Radio Emission ◽  
Supernova Remnants ◽  
Angular Resolution ◽  
Angular Size ◽  
Cosmic Ray ◽  
Lebedev Physical Institute ◽  
Physical Institute ◽  
Contour Maps ◽  
Lebedev Physical

Contour maps at 102· 5 MHz for 12 galactic SNRs of large angular size in the northern sky are presented. The observations were made with an angular resolution of 48' x24' sec(55° - 8) using the BSA telescope of the Lebedev Physical Institute. All sources were mapped in total intensity. Our results indicate that the contribution to the radiation of observed SNRs from swept up cosmic ray electrons is small. The characteristics of the observed sources are discussed.

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