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Table A.1.

Convective shifts of spectral lines in the quiet Sun.

Spectral line Line R Heliocentric position μ = cosθ
(λ0 in Å) section 1.0 0.95 0.9 0.85 0.8 0.7 0.6 0.5 0.4 0.3 0.2
Fe I 5250.2084 Full 700 000 −226 −286 −241 −346 −300 −271 −253 −237 −226 −157 −7
Core 700 000 −99 −191 −170 −286 −251 −222 −190 −162 −132 −38 111
250 000 −141 −222 −193 −303 −264 −233 −201 −174 −145 −52 96
180 000 −169 −243 −210 −315 −274 −242 −210 −184 −157 −64 83
100 000 −221 −283 −241 −342 −297 −263 −235 −211 −188 −101 46
Fe I 5250.6453 Full 700 000 −274 −318 −257 −349 −287 −236 −202 −170 −147 −69 89
Core 700 000 −74 −126 −80 −180 −126 −82 −32 10 52 144 268
250 000 −113 −165 −116 −212 −157 −109 −59 −15 27 120 250
180 000 −145 −197 −146 −239 −182 −131 −81 −37 5 99 234
100 000 −228 −276 −219 −307 −247 −191 −144 −101 −61 34 180
C I 5380.3308 Full 700 000 −1028 −988 −974 −940 −959 −887 −802 −764 −708 −679
Core 700 000 −1015 −980 −977 −935 −950 −890 −796 −783 −738 −688
250 000 −1022 −986 −981 −940 −957 −898 −808 −785 −742 −714
180 000 −1027 −990 −983 −944 −962 −901 −814 −788 −743 −718
100 000 −1040 −1000 −989 −953 −973 −906 −821 −790 −743 −719
Fe I 5434.5232 Full 700 000 −179 −204 −175 −242 −178 −211 −172 −103 −40 22 115
Core 700 000 1 −2 16 −4 55 39 90 181 225 269 321
250 000 −15 −21 −1 −24 36 20 72 165 211 258 312
180 000 −32 −39 −19 −44 17 1 55 149 197 247 302
100 000 −93 −106 −81 −114 −50 −67 −6 87 145 203 265
Fe I 5432.9470 Full 700 000 −312 −357 −313 −397 −337 −381 −341 −289 −222 −171 −74
Core 700 000 −217 −277 −249 −331 −274 −323 −276 −208 −140 −77 −5
250 000 −237 −292 −261 −342 −284 −332 −284 −218 −149 −84 −7
180 000 −253 −305 −271 −351 −292 −339 −290 −226 −156 −91 −10
100 000 −292 −338 −298 −378 −316 −360 −312 −249 −180 −115 −24
Fe I 5576.0881 Full 700 000 −158 −166 −160 −108 −150 −110 −91 −54 −17 37 98
Core 700 000 −31 −47 −36 0 −33 1 22 68 81 131 140
250 000 −59 −75 −63 −23 −56 −18 7 55 72 125 139
180 000 −84 −98 −85 −42 −75 −34 −7 43 63 119 138
100 000 −150 −159 −145 −95 −128 −80 −47 4 34 98 132
Na I 5895.92424 Full 700 000 −99 −110 −81 −101 −84 −78 −33 −42 11 19 37
Core 700 000 32 18 35 9 45 26 61 51 65 45 52
250 000 30 15 31 7 43 25 59 48 65 45 47
180 000 27 12 29 5 41 24 58 47 64 44 45
100 000 19 3 23 −2 34 20 56 43 62 43 41
Fe II 6149.2460 Full 700 000 −430 −425 −392 −379 −404 −381 −392 −320 −296 −215 −142
Core 700 000 −412 −429 −405 −385 −409 −396 −391 −296 −261 −180 −63
250 000 −430 −441 −413 −393 −417 −399 −396 −304 −270 −184 −80
180 000 −443 −450 −419 −398 −422 −401 −398 −309 −275 −188 −90
100 000 −464 −462 −427 −406 −429 −404 −404 −320 −287 −201 −113
Fe I 6173.3344 Full 700 000 −262 −309 −257 −280 −242 −205 −233 −258 −151 −75
Core 700 000 −177 −243 −208 −239 −210 −169 −186 −191 −63 29
250 000 −207 −267 −228 −254 −221 −180 −197 −204 −77 14
180 000 −228 −285 −241 −265 −230 −189 −206 −214 −88 2
100 000 −267 −317 −267 −287 −249 −208 −227 −242 −119 −31
81 000 −275 −322 −271 −291 −252 −212 −234 −251 −132 −46
Fe I 6301.5008 Full 700 000 −295 −242 −255 −270 −229 −269 −254 −203 −155 −86
Core 700 000 −110 −73 −90 −108 −70 −104 −69 −19 29 82
250 000 −137 −98 −113 −131 −90 −123 −86 −33 18 76
180 000 −161 −120 −133 −150 −107 −139 −101 −46 8 69
100 000 −229 −183 −192 −206 −158 −188 −149 −89 −28 43
Fe I 6302.4932 Full 700 000 −293 −245 −259 −280 −236 −281 −272 −219 −170 −96
Core 700 000 −164 −136 −168 −199 −161 −204 −176 −116 −53 28
250 000 −195 −163 −189 −218 −178 −220 −191 −130 −66 16
180 000 −219 −184 −206 −233 −191 −232 −203 −142 −78 6
100 000 −276 −233 −248 −269 −225 −264 −237 −176 −113 −27

Notes. The Doppler velocities (in m s−1) from the disk center (μ = 1.0) to the solar limb (μ = 0.2) are listed for different spectral resolutions R. Average velocities are given for the full line profile (from the line minimum to an upper threshold close to the continuum intensity level) and only the line core (lower 5% of the bisector).

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