WebSVN – svnkaklik – Diff – //dokumenty/skolni/diplomka/introduction.tex



 
Today radioastronomy knows several observation types.
 
\begitems
* Spectral observations
* Intensity observations
* Velocity observations
\enditems
 
All of these observations ideally needs high frequency resolution and stability. Wide observation bandwidth in hundreds of MHz is usually desirable for easier discrimination of source types. 
 

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13	`Today radioastronomy knows several observation types.`	13	`Today radioastronomy knows several observation types.`
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15	`\begitems`	15	`\begitems`
16	`* Spectral observations`	16	`* Spectral observations`
17	`* Instensity observations`	17	`* Intensity observations`
18	`* Velocity observations`	18	`* Velocity observations`
19	`\enditems`	19	`\enditems`
20		20
21	`All of these observations ideally needs high frequency resolution and stability. Wide observation bandwidth in hundreds of MHz is usually desirable for easier discrimination of source types.`	21	`All of these observations ideally needs high frequency resolution and stability. Wide observation bandwidth in hundreds of MHz is usually desirable for easier discrimination of source types.`
22		22

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(root)//dokumenty/skolni/diplomka/introduction.tex – Rev 1085 → 1086