... java.lang.Object ij.gui.Roi ij.gui.Line . ... public class Line . ... int . ... protected double . ... Constructor Detail public Line (int ox1, int oy1, int ox2, int oy2) . Creates a new straight line selection using the specified starting and ending offscreen integer coordinates. public Line (double ox1, double oy1, double ox2, double oy2) . Creates a new straight line selection using the specified starting and ending offscreen double coordinates. public Line (int sx, int sy, ImagePlus imp) . ...

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• Uses of Class ij.gui.Line (ImageJ API)
• Wand (ImageJ API)
• Plot (ImageJ API)

... Here we will look at line plots. We will go through steps, such as changing linestyles and symbols, you can use to modify your line plots. ... IDL> plot, num, line . ... IDL> plot, num, line, psym = 1 . ... IDL> plot, num, line, linestyle = 1 . ... Line Style . ... IDL> plot, num, line, linestyle=2, thick=3 . ... IDL> plot, num, line, psym = 8, symsize = 2.0 . ... IDL> plot, num, line, charsize=2.0, title='GHRS spectrum . ... IDL> plot, num, line, charsize=2.0, xcharsize=0.8, xtitle='wavelength' . ...

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• The Continuum and Line Spectra of the Seyfert 2 Galaxy NGC 5252: Radiation and
• STScI On-line Conference Proceedings
• Emission Line

... As a result of BTA observations of 23 chemically peculiar stars with strong magnetic fields, it was found that in 22 of them the longitudinal magnetic field, measured from the hydrogen line cores are considerably lower (by about 1/3) than the value measured from metal lines in the same spectra. ... New approaches need to be developed in order to interpret the data. ... The Zeeman spectrum of a star with a strong magnetic field, 53 Cam. ...

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• V1494
• Figure 1
• Solar system sector, archive 1998

... Upper 2{sigma} error in GammaUV 25- 29 F5.2 --- e_GammaUV ? ... GammaUV is fitted at {lambda}_rest_<4200{AA}. ... ------------------------------------------------------------------------ 1- 11 A11 --- NSpect Spectrum name (G1) 14- 19 I6 km/s FWHM _ly Rest frame Full Width at Half Maximum of total Lya 22- 27 I6 km/s E_FWHM Upper 2{ sigma } error limit on FWHM of total Lya 30- 35 I6 km/s e_FWHM Lower 2{ sigma } error limit on FWHM of total Lya 38- 43 I6 km/s FWHM _c4 ...

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• http://hea-www.harvard.edu/~pgreen/Papers/DATA/post_FOS_WWW/notes_to_electronic_tables
• The AstroStat Slog line
• The AstroStat Slog emission line

... Magnetic field lines similarly describe the structure of magnetic fields in three dimensions.They are defined as follows. If at any point on such a line we place an ideal compass needle, free to turn in any direction (unlike the usual compass needle, which stays horizontal) then the needle will always point along the field line (drawing below). Field lines converge where the magnetic force is strong , and spread out where it is weak. ... Exploration" home page (index) Glossary . ...

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• Magnetic Field Lines -- History
• Power line harmonics [Oulu]
• Principles of the Magnetic Trapping of Particles