H. Neckel

2.3k total citations · 1 hit paper
42 papers, 1.6k citations indexed

About

H. Neckel is a scholar working on Astronomy and Astrophysics, Atmospheric Science and Aerospace Engineering. According to data from OpenAlex, H. Neckel has authored 42 papers receiving a total of 1.6k indexed citations (citations by other indexed papers that have themselves been cited), including 26 papers in Astronomy and Astrophysics, 10 papers in Atmospheric Science and 8 papers in Aerospace Engineering. Recurrent topics in H. Neckel's work include Solar and Space Plasma Dynamics (23 papers), Atmospheric Ozone and Climate (10 papers) and Stellar, planetary, and galactic studies (8 papers). H. Neckel is often cited by papers focused on Solar and Space Plasma Dynamics (23 papers), Atmospheric Ozone and Climate (10 papers) and Stellar, planetary, and galactic studies (8 papers). H. Neckel collaborates with scholars based in Germany, France and United States. H. Neckel's co-authors include D. Labs, P. Esquinazi, Ernst Helmut Brandt, G. Weiß, G. Thuillier, Pierre Simon, Siegfried Hunklinger, J. Wolfrum, A. Greve and P. Monkhouse and has published in prestigious journals such as Nature, Science and Physical Review Letters.

In The Last Decade

H. Neckel

40 papers receiving 1.4k citations

Hit Papers

align trajectories

What are hit papers?

Hit papers significantly outperform the citation benchmark for their cohort. A paper qualifies if it has ≥500 total citations, achieves ≥1.5× the top-1% citation threshold for papers in the same subfield and year (this is the minimum needed to enter the top 1%, not the average within it), or reaches the top citation threshold in at least one of its specific research topics.

The solar radiation between 3300 and 12500 �

1984 611 citations H. Neckel, D. Labs Solar Physics profile →

Peers — A (Enhanced Table)

Peers by citation overlap · career bar shows stage (early→late) cites · hero ref

Name	h						Papers	Cites
H. Neckel Germany	17	680	530	362	285	204	42	1.6k
R. L. Huguenin Switzerland	20	640 0.9×	227 0.4×	118 0.3×	118 0.4×	144 0.7×	87	1.2k
Frédéric Moisy France	24	365 0.5×	216 0.4×	175 0.5×	109 0.4×	101 0.5×	52	1.7k
U. Klein Germany	17	70 0.1×	414 0.8×	370 1.0×	169 0.6×	318 1.6×	79	1.4k
Hideaki Nakane Japan	20	129 0.2×	784 1.5×	675 1.9×	63 0.2×	193 0.9×	124	1.4k
Steven W. Brown United States	24	82 0.1×	618 1.2×	292 0.8×	909 3.2×	118 0.6×	132	2.4k
Patrice Le Gal France	31	541 0.8×	250 0.5×	177 0.5×	318 1.1×	142 0.7×	102	2.5k
Yves Tessier France	18	172 0.3×	275 0.5×	577 1.6×	231 0.8×	48 0.2×	37	1.6k
Walter G. Egan United States	18	189 0.3×	155 0.3×	221 0.6×	144 0.5×	26 0.1×	76	826
Hongbo Zhang China	23	1.2k 1.8×	134 0.3×	387 1.1×	181 0.6×	116 0.6×	87	1.6k
Y. Yokota Japan	32	2.4k 3.5×	543 1.0×	36 0.1×	674 2.4×	55 0.3×	132	3.0k

Countries citing papers authored by H. Neckel

Since Specialization

Citations

This map shows the geographic impact of H. Neckel's research. It shows the number of citations coming from papers published by authors working in each country. You can also color the map by specialization and compare the number of citations received by H. Neckel with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites H. Neckel more than expected).

Fields of papers citing papers by H. Neckel

Since Specialization

Physical SciencesHealth SciencesLife SciencesSocial Sciences

This network shows the impact of papers produced by H. Neckel. Nodes represent research fields, and links connect fields that are likely to share authors. Colored nodes show fields that tend to cite the papers produced by H. Neckel. The network helps show where H. Neckel may publish in the future.

Co-authorship network of co-authors of H. Neckel

This figure shows the co-authorship network connecting the top 25 collaborators of H. Neckel. A scholar is included among the top collaborators of H. Neckel based on the total number of citations received by their joint publications. Widths of edges represent the number of papers authors have co-authored together. Node borders signify the number of papers an author published with H. Neckel. H. Neckel is excluded from the visualization to improve readability, since they are connected to all nodes in the network.

All Works

Sort: Min cites: Since: Top N: Style:

20 of 20 papers shown

1.

Fernley, J. A., H. Neckel, E. Solano, & W. Wamsteker. (1996). A study of solar analogues in the ultraviolet.. 311(1). 245–252. 2 indexed citations

2.

Neckel, H.. (1995). The solar radius derived from limb-darkening scans obtained in 1981 and from 1986 to 1990. Solar Physics. 156(1). 7–16. 21 indexed citations

3.

Neckel, H. & D. Labs. (1994). Solar limb darkening 1986–1990 (λλ303 to 1099 nm). Solar Physics. 153(1-2). 91–114. 125 indexed citations

4.

Wolfrum, J., et al.. (1991). In situ measurement of ammonia concentration in industrial combustion systems. Symposium (International) on Combustion. 23(1). 231–236. 8 indexed citations

5.

Neckel, H. & D. Labs. (1990). The role of telescopic stray light in limb-darkening scans obtained in April 1981 (and later). Solar Physics. 126(1). 47–52. 2 indexed citations

6.

Arnold-Bos, Andreas, H. Becker, W. Hentschel, et al.. (1990). Laser in situ monitoring of combustion processes. Applied Optics. 29(33). 4860–4860. 33 indexed citations

7.

Neckel, H. & D. Labs. (1989). Multiplier hysteresis and image motion errors in limb darkening scans obtained in April 1981 (and later). Solar Physics. 120(1). 205–207. 10 indexed citations

8.

Neckel, H. & D. Labs. (1987). Asymmetry and variations of solar limb darkening along the diameter defined by diurnal motion in April 1981. Solar Physics. 110(1). 139–170. 12 indexed citations

9.

Labs, D., H. Neckel, Pierre Simon, & G. Thuillier. (1987). Ultraviolet solar irradiance measurement from 200 to 358 nm during spacelab 1 mission. Solar Physics. 107(2). 203–219. 47 indexed citations

10.

Esquinazi, P., H. Neckel, G. Weiß, & Ernst Helmut Brandt. (1986). A superconducting vibrating reed applied to flux-line pinning. II. Experiment. Journal of Low Temperature Physics. 64(1-2). 1–20. 42 indexed citations

11.

Neckel, H.. (1986). The Bright Stars with UBV-colors close to those of the sun. 169. 194–200. 4 indexed citations

12.

Esquinazi, P., et al.. (1986). Acoustic experiments on amorphous Pd30Zr70 and Cu30Zr70 in the superconducting and the normal state. The European Physical Journal B. 64(1). 81–93. 43 indexed citations

13.

Brandt, Ernst Helmut, et al.. (1986). Drastic increases of frequency and damping of a superconducting vibrating reed in a longitudinal magnetic field. Physical Review Letters. 56(1). 89–92. 63 indexed citations

14.

Neckel, H. & D. Labs. (1984). The solar radiation between 3300 and 12500 �. Solar Physics. 90(2). 611 indexed citations breakdown →

15.

Neckel, H.. (1984). Recent improvements of the basic solar radiation data for ?? 3300-12500 �. Space Science Reviews. 38(3-4). 2 indexed citations

16.

Neckel, H. & D. Labs. (1981). Improved data of solar spectral irradiance from 0.33 to 1.25?. Solar Physics. 74(1). 231–249. 135 indexed citations

17.

Thuillier, G., et al.. (1981). An instrument to measure the solar spectrum from 170 to 3200 nm on board Spacelab. Solar Physics. 74(2). 531–537. 16 indexed citations

18.

Labs, D. & H. Neckel. (1971). The solar constant. Solar Physics. 19(1). 3–15. 13 indexed citations

19.

Labs, D. & H. Neckel. (1970). Transformation of the absolute solar radiation data into the ?International Practical Temperature Scale of 1968?. Solar Physics. 15(1). 79–87. 111 indexed citations

20.

Labs, D. & H. Neckel. (1968). The Radiation of the Solar Photosphere from 2000 Å to 100 μm. 69. 1. 16 indexed citations

Rankless uses publication and citation data sourced from OpenAlex, an open and comprehensive bibliographic database. While OpenAlex provides broad and valuable coverage of the global research landscape, it—like all bibliographic datasets—has inherent limitations. These include incomplete records, variations in author disambiguation, differences in journal indexing, and delays in data updates. As a result, some metrics and network relationships displayed in Rankless may not fully capture the entirety of a scholar's output or impact.

Explore authors with similar magnitude of impact