274:
22:
161:
Heliospheric imagers are generally flown in space because the Earth's atmosphere itself interferes with the signal even at night. Terrestrial features such as clouds, aircraft, moonlight, small variations in dust and moisture content of the air column, and even high altitude
154:. Heliospheric imagers are simple in principle โ they are simple visible light cameras placed inside deep optical baffles. However, the solar wind features are extremely faint โ as little as 0.1% of the brightness of the background starfield and
178:
spacecraft in deep space. The concept was first demonstrated in the 1980s via detailed post-processing of photometer data from the two HELIOS spacecraft flown in the 1970s.
86:
170:, can obscure the desired solar wind signal. Instruments flown to date include the Solar Mass Ejection Imager (SMEI) flown on a
58:
65:
39:
315:
174:
satellite in high polar orbit, and the HI imagers that formed part of the SECCHI instrument suite on board NASA's twin
105:
72:
158: โ and therefore heliospheric imager data require extensive post-processing to remove these backgrounds.
54:
43:
273:
79:
32:
339:
334:
308:
289:
243:
204:
8:
216:
247:
208:
344:
147:
301:
251:
212:
135:
285:
155:
256:
231:
328:
151:
123:
232:"Sun Earth Connection Coronal and Heliospheric Investigation (SECCHI)"
143:
21:
163:
175:
167:
146:. The electrons, in particular, scatter incident sunlight via
195:
Eyles, C. J. (2003). "The Solar Mass
Ejection Imager (Smei)".
171:
150:, and clouds of plasma can therefore be photographed using
281:
139:
122:
is a wide-field camera that is designed to image the
126:in interplanetary space, far from the Sun itself.
46:. Unsourced material may be challenged and removed.
326:
309:
316:
302:
255:
106:Learn how and when to remove this message
327:
229:
194:
268:
44:adding citations to reliable sources
15:
13:
217:10.1023/B:SOLA.0000006903.75671.49
14:
356:
272:
20:
31:needs additional citations for
223:
188:
134:The solar wind is composed of
1:
181:
288:. You can help Knowledge by
280:This article related to the
7:
129:
10:
361:
267:
257:10.1007/s11214-008-9341-4
230:Howard, R. A. (2008).
236:Space Science Reviews
55:"Heliospheric imager"
40:improve this article
248:2008SSRv..136...67H
209:2003SoPh..217..319E
120:heliospheric imager
148:Thomson scattering
138:and contains both
297:
296:
116:
115:
108:
90:
352:
318:
311:
304:
276:
269:
262:
261:
259:
227:
221:
220:
192:
111:
104:
100:
97:
91:
89:
48:
24:
16:
360:
359:
355:
354:
353:
351:
350:
349:
325:
324:
323:
322:
266:
265:
228:
224:
193:
189:
184:
132:
112:
101:
95:
92:
49:
47:
37:
25:
12:
11:
5:
358:
348:
347:
342:
337:
321:
320:
313:
306:
298:
295:
294:
277:
264:
263:
222:
186:
185:
183:
180:
156:zodiacal light
131:
128:
114:
113:
28:
26:
19:
9:
6:
4:
3:
2:
357:
346:
343:
341:
340:Space imagers
338:
336:
335:Space weather
333:
332:
330:
319:
314:
312:
307:
305:
300:
299:
293:
291:
287:
283:
278:
275:
271:
270:
258:
253:
249:
245:
241:
237:
233:
226:
218:
214:
210:
206:
202:
198:
197:Solar Physics
191:
187:
179:
177:
173:
169:
165:
159:
157:
153:
152:visible light
149:
145:
141:
137:
127:
125:
121:
110:
107:
99:
88:
85:
81:
78:
74:
71:
67:
64:
60:
57: โ
56:
52:
51:Find sources:
45:
41:
35:
34:
29:This article
27:
23:
18:
17:
290:expanding it
279:
239:
235:
225:
203:(Nov): 319.
200:
196:
190:
160:
133:
119:
117:
102:
93:
83:
76:
69:
62:
50:
38:Please help
33:verification
30:
242:(1โ4): 67.
329:Categories
182:References
124:solar wind
66:newspapers
345:Sun stubs
144:electrons
142:and free
96:June 2017
130:Overview
244:Bibcode
205:Bibcode
164:airglow
80:scholar
176:STEREO
168:aurora
136:plasma
82:
75:
68:
61:
53:
284:is a
87:JSTOR
73:books
286:stub
172:USAF
166:and
140:ions
59:news
282:Sun
252:doi
240:136
213:doi
201:217
42:by
331::
250:.
238:.
234:.
211:.
199:.
118:A
317:e
310:t
303:v
292:.
260:.
254::
246::
219:.
215::
207::
109:)
103:(
98:)
94:(
84:ยท
77:ยท
70:ยท
63:ยท
36:.
Text is available under the Creative Commons Attribution-ShareAlike License. Additional terms may apply.