Sa. Suleymanova et al., INDIVIDUAL AND INTEGRATED PULSE PROPERTIES OF PSR B0943-CHANGING PHENOMENON(10 INVOLVED IN THE MODE), Journal of astrophysics and astronomy, 19(1-2), 1998, pp. 1-18
The characteristics of the ''burst'' (B) mode and ''quiescent'' (Q) mo
de pulse sequences-long known from studies at or below 103 MHz-are ide
ntified at 430MHz for the first time. An 18-minute, polarimetric obser
vation begins with a long B-mode sequence, which has a higher average
intensity, regular drifting subpulses, and a preponderance of primary
polarisation-mode radiation. An abrupt transition to a Q-mode sequence
is then marked by a) weaker average intensity, but occasional very br
ight individual subpulses: b) a complete cessation of drifting subpuls
es, with disorganized subpulses now being emitted over a much wider lo
ngitude interval, and c) near parity between the primary and secondary
polarisation modes, resulting in pronounced depolarisation, both of i
ndividual pulses and the average profile. Careful study, however, of p
rofile changes before and after this mode change reveals slower variat
ions which both anticipate the abrupt transition and respond to it. A
slow attenuation of the intensity level of the dominant component is o
bserved throughout the duration of the B-mode sequence, which then acc
elerates with the onset of the Q-mode sequence. This slow variation ap
pears to represent a ''pre-switching transition'' process; and the com
bination of effects on slow and abrupt time scales are finally respons
ible for the formation of the characteristic B- and Q-mode average pro
files.