Latest Images

Left panel (a): The 3.0–14.5 μm spectra of regi...

Left panel (a): The 3.0–14.5 μm spectra of regions 0–13 (from bottom to top), normalized...

Junhao Peng et al, The Astrophysical Journal 1010 1

(a) The JWST/NIRSpec and MIRI spectrum of Regio...

(a) The JWST/NIRSpec and MIRI spectrum of Region 1 is decomposed with PAHFIT. (b) Zoomed...

Junhao Peng et al, The Astrophysical Journal 1010 1

Zoomed-in view of the PAHFIT decomposition arou...

Zoomed-in view of the PAHFIT decomposition around 6.85 μm for the R2–R13 regions. The 6....

Junhao Peng et al, The Astrophysical Journal 1010 1

Zoomed-in view of the PAHFIT decomposition arou...

Zoomed-in view of the PAHFIT decomposition around 3.3 μm for the R2–R13 regions.

Junhao Peng et al, The Astrophysical Journal 1010 1

JWST’s MIRI IFU slice at 6.2 μm for the 30 Dora...

JWST’s MIRI IFU slice at 6.2 μm for the 30 Doradus star-forming complex in the LMC. R0–R...

Junhao Peng et al, The Astrophysical Journal 1010 1

Pixel-by-pixel map of the aliphatic to aromatic...

Pixel-by-pixel map of the aliphatic to aromatic C–H band ratio (I3.4/I3.3), with the ape...

Junhao Peng et al, The Astrophysical Journal 1010 1

PAHFIT analysis of Region R3. The left panel is...

PAHFIT analysis of Region R3. The left panel is for the full spectrum, while the right p...

Junhao Peng et al, The Astrophysical Journal 1010 1

Left panel (a): relation between the 3.4 μm ali...

Left panel (a): relation between the 3.4 μm aliphatic C–H stretch and the 6.85 μm alipha...

Junhao Peng et al, The Astrophysical Journal 1010 1

Local spectral decomposition of the 4.65 and 4....

Local spectral decomposition of the 4.65 and 4.75 μm aliphatic C–D bands for Regions R2–...

Junhao Peng et al, The Astrophysical Journal 1010 1

Relation between the 3.4 μm aliphatic C–H stret...

Relation between the 3.4 μm aliphatic C–H stretch and the 4.65 μm aliphatic C–D stretch....

Junhao Peng et al, The Astrophysical Journal 1010 1

Top panels show the magnetic-field components, ...

Top panels show the magnetic-field components, magnetic-field magnitude (left y-axis), a...

Sofiane Bourouaine, The Astrophysical Journal Letters 1010 1

The top and middle rows show the distributions ...

The top and middle rows show the distributions of the local estimates of the mixed third...

Sofiane Bourouaine, The Astrophysical Journal Letters 1010 1

Ensemble-averaged structure functions associate...

Ensemble-averaged structure functions associated with outward (...

Sofiane Bourouaine, The Astrophysical Journal Letters 1010 1

Power spectral densities of the outward, Pout (...

Power spectral densities of the outward, Pout (top panel), and inward, Pin (bottom panel...

Sofiane Bourouaine, The Astrophysical Journal Letters 1010 1

Identification of the dimming source region and...

Identification of the dimming source region and comparison between AIA and EVE light cur...

Xinyue Wang et al, The Astrophysical Journal Letters 1010 1

Evolution of the M8.8 flare on 2012 July 5. The...

Evolution of the M8.8 flare on 2012 July 5. The top and second rows show the side-on vie...

Xinyue Wang et al, The Astrophysical Journal Letters 1010 1

Overview of the M8.8 confined flare on 2012 Jul...

Overview of the M8.8 confined flare on 2012 July 5. (a) GOES SXR flux in the 1–8 Å and 0...

Xinyue Wang et al, The Astrophysical Journal Letters 1010 1

Thermal evolution and plasma cooling during the...

Thermal evolution and plasma cooling during the confined flare. All AIA quantities are d...

Xinyue Wang et al, The Astrophysical Journal Letters 1010 1

AIA 94 Å images showing persistent high-tempera...

AIA 94 Å images showing persistent high-temperature loop emission in the core of NOAA 11...

Xinyue Wang et al, The Astrophysical Journal Letters 1010 1

Long-term light curves of GOES 0.5–4 Å, GOES 1–...

Long-term light curves of GOES 0.5–4 Å, GOES 1–8 Å, EVE Fe XX 13.29 nm, AIA 131 Å, EVE F...

Xinyue Wang et al, The Astrophysical Journal Letters 1010 1

One-dimensional y-averaged profile for density ...

One-dimensional y-averaged profile for density (top), x-directional three-velocity (seco...

Kazuki Kamiido and Yutaka Ohira, The Astrophysical Journal Letters 1010 1

Two-dimensional profile at tωpe = 600 for the d...

Two-dimensional profile at tωpe = 600 for the density (top) and the x, y, and z-componen...

Kazuki Kamiido and Yutaka Ohira, The Astrophysical Journal Letters 1010 1

Power spectrum of the x-component of the magnet...

Power spectrum of the x-component of the magnetic field at x/(c/ωpe) = 0 shown for each ...

Kazuki Kamiido and Yutaka Ohira, The Astrophysical Journal Letters 1010 1

The same as Figure 2, but zooming into 50 < x/(...

The same as Figure 2, but zooming into 50 < x/(c/ωpe) < 350 and the magnetic field is Lo...

Kazuki Kamiido and Yutaka Ohira, The Astrophysical Journal Letters 1010 1

Phase space in the upstream rest frame at tωpe ...

Phase space in the upstream rest frame at tωpe = 600.

Kazuki Kamiido and Yutaka Ohira, The Astrophysical Journal Letters 1010 1

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Updated Search and Sort

We have updated the search and sort algorithm to return records in reverse chronological order based on the date/time that the images were uploaded to the Astronomy Image Explorer. This is potentially but rarely different from the publication date. Thank you!