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<journal-id journal-id-type="publisher">london-journal-of-research-in-science-natural-and-formal</journal-id>
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<journal-title>London Journal of Research In Science: Natural and Formal</journal-title>
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<issn publication-format="print">2631-8490</issn>
<issn publication-format="electronic">2631-8504</issn>
<publisher><publisher-name>JournalsPress</publisher-name></publisher>
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<article-id pub-id-type="publisher-id">66164</article-id>
<title-group>
<article-title>Pulsars in Radio Wave</article-title>
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<volume>19</volume>
<issue>7</issue>
<fpage>17</fpage>
<lpage>19</lpage>
<abstract><p>This paper will utilize a methodological approach to determine the precise period of a pulsar and calculate the distance of the pulsar. Because the period of a pulsar changes depending on the time of year the observation is collected, a precise period needs to be calculated from the raw period. The distance of a pulsar can be calculated based on the signal??s time delay due to the interstellar medium. Because the noise in the data is extremely strong compared to the signal, it is necessary to collect data using different channels; the signal from the pulsar can be determined by adding the signal in each every channel and calculating the average signal value.</p></abstract>
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<p>This paper will utilize a methodological approach to determine the precise period of a pulsar and calculate the distance of the pulsar. Because the period of a pulsar changes depending on the time of year the observation is collected, a precise period needs to be calculated from the raw period. The distance of a pulsar can be calculated based on the signal??s time delay due to the interstellar medium. Because the noise in the data is extremely strong compared to the signal, it is necessary to collect data using different channels; the signal from the pulsar can be determined by adding the signal in each every channel and calculating the average signal value.</p>
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