Note on terminology: large spicules seen at the limb in coronal
holes are often called macro-spicules, usually if they have a
transition region component. However, if they also have a coronal
component (say Ne VIII from SUMER, or Mg IX from CDS) then I consider
these to be coronal jets.
| Paper |
Comments |
| Pike &
Harrison (1997, Sol.
Phys.) |
Macrospicule at CH limb with Mg
IX signature; velocity increased with height. |
| Pike &
Mason (1998, Sol. Phys.) |
Presented 6 macrospicules, 5 of
which had Mg IX signature; all showed evidence of rotation. |
| Banerjee et
al. (2000, A&A, 355, 1152) |
Macrospicule sit-and-stare
observation, with coronal signature. |
| Parenti et
al. (2002, A&A) |
Macrospicule raster observation,
but no coronal signature. |
| Paper |
Comments |
| Wilhelm
(2000, A&A) |
Study of spicules and
macrospicules; one macrospicule did not show a coronal signature (Mg
X); LOS velocities are about 30 km/s. |
| Wilhelm et
al. (2002, Ap.&SS, 282, 189) |
Single jet in CH close to south
limb; seen in Ne VIII & C IV; raster scan. |
| Xia et al.
(2005, A&A 438, 1115) |
Two macrospicules;
sit-and-stare; no hot plasma reported; MS consist of multiple spicules. |
| Popescu et
al. (2007, Adv.Sp.Res., 40, 1021) |
Macrospicule seen at limb in Ne
VIII; sit-and-stare; MS above limb; 10 km/s. Explosive event also
presented, and looks like jet. |
| Madjarska et
al. (2007, ApJ, 670, L57) |
3 features that look like jets
in the core of active region observed by TRACE; SUMER shows red-shifts
in O V and Mg X; features probably downflows along closed loops. |
| Scullion et
al. (2009, ApJ, 704, 1385) |
4
jets in polar coronal holes (off-limb and on-disk); the only clear
coronal jet is the same one studied by Popescu et al. (2007) |
| Gontikakis
et al. (2009, A&A, 506, L45) |
Small active region jet seen
with TRACE and SUMER (Ne VIII & C IV); due to emerging flux;
velocity around 120 km/s; compared with a model. |
| Kamio et al. (2010, A&A, 510, 1) | X-ray jet (XRT) that shows a macrospicule (EUVI, 304); observed by both EIS and SUMER; jet is at limb. |
| Madjarska et al. (2011, A&A, 526, 19) | Jet at boundary of an equatorial
coronal hole; observed by XRT, EIS, SUMER and EUVI; |
| Curdt &
Tian (2011, A&A) |
Presented two explosive events
near sunspot, but in discussion showed nice example of a rotating
macrospicule above the limb in O V 629.7. |
| Paper |
Comments |
| Culhane et
al. (2007, PASJ, 59, 745) |
Two CH jets seen in slot data;
suggests material falls back to the Sun. |
| Kamio et al.
(2007, PASJ, 59, 751) |
CH jet seen in one raster; LOS
velocity of 30 km/s in Fe XII (may be higher if background was
subtracted); BP is quite large. |
| Kim et al. (2007, PASJ, 59, 763) |
AR jet from 28-Jan-2007 near limb; EIS observed bright point during ejection. |
| Moreno-Insertis
et al. (2008, ApJL, 673, 211) |
Jet in eq. CH; sit-and-stare;
slit crosses perpendicular to jet; finds distinct jet component at 240
km/s; density is 5.5x10^9 cm^-3. |
| Chifor et
al. (2008, A&A, 481, L57) |
AR jet on disk; velocities up to
150 km/s; high densities (10^11) |
| Kamio et
al. (2009, A&A, 502, 345) |
EIS & SUMER; on-disk coronal
hole; 6 jets observed by EIS (Fe XII) |
| Doschek et al. (2010, ApJ) |
On-disk polar coronal hole jet |
| Sterling et
al. (2010, ApJ, 72, 1644) |
Jet in north coronal hole at
limb; seen with 266" slot; cool material (He II 256; SOT) mixed with
hot material (Fe XV; XRT); interpreted as blowout jet |
| Kamio et
al. (2010, A&A, 510, 1) |
X-ray jet (XRT) that shows a
macrospicule (EUVI, 304); observed by both EIS and SUMER; jet is at
limb. |
| Madjarska
et al. (2011, A&A, 526, 19) |
CH jet |
| Yang et al. (2011, RAA, 11, 1229) |
Three AR jets from AR 10960 (5-Jun-2007). |
| Matsui et al.
(2012, ApJ, 759, 15) |
AR jet from 5-Jun-2007 (the middle jet of Yang et al. 2011); jet seen up to Fe XVI; extends to 60 Mm. |
| Tian et al. (2012, ApJ, 748, 106) |
Discusses the first two AR jets from Yang et al. (2011) |
| Lee et al.
(2013, ApJ, 766, 1) |
AR jet at limb (SDO and EIS);
EIS sit-and-stare; mainly seen in cool temps (He II); Fe XII shows
dimming signature. |
| Chandrasekhar
et al. (2014, A&A, 561, 104) |
Two
polar coronal hole jets; one observed by EIS in 40" slot data. Derived
speed of about 170 km/s in Fe XII. Lateral motion of jet is highlighted. |
| Young &
Muglach (2014, Sol. Phys., 289, 3313) |
|
| Young &
Muglach (2014, PASJ, 66, 12) |
| Paper |
Comments |
| Cheung et al. (2015, ApJ, 801, 83) |
Homologous active region jets observed with IRIS and SDO; find evidence from twist |