2019
DOI: 10.3389/fnagi.2019.00345
|View full text |Cite
|
Sign up to set email alerts
|

White Matter Regions With Low Microstructure in Young Adults Spatially Coincide With White Matter Hyperintensities in Older Adults

Help me understand this report

Search citation statements

Order By: Relevance

Paper Sections

Select...
3

Citation Types

0
3
0

Year Published

2020
2020
2024
2024

Publication Types

Select...
3

Relationship

1
2

Authors

Journals

citations
Cited by 3 publications
(3 citation statements)
references
References 47 publications
(62 reference statements)
0
3
0
Order By: Relevance
“…The increase in WMH with age is well documented in the general population (95-96% of those aged >60 years 45,46 and 100% of those aged >65 years 47 in the general population). In these adults with DS, 100% had detectable WMH (range = 0.01-23.0cm 3 ).…”
Section: Discussionmentioning
confidence: 91%
“…The increase in WMH with age is well documented in the general population (95-96% of those aged >60 years 45,46 and 100% of those aged >65 years 47 in the general population). In these adults with DS, 100% had detectable WMH (range = 0.01-23.0cm 3 ).…”
Section: Discussionmentioning
confidence: 91%
“…Our results support a robust relation between genetic determinants of WMH, the most common imaging feature of cSVD in older adults, and NODDI markers, especially NDI, in young adults. Interestingly, associations of genetically predicted WMH with NDI markers at age 20 were observed primarily in white matter regions most commonly affected by WMH in older age [90,91], such as the anterior, posterior and superior corona radiata, posterior thalamic radiation, and superior longitudinal fasciculus. This corroborates recent observations that areas where WMH are most likely to appear in older adults are also those with the lowest white matter microstructure integrity on DTI in young adults [91].…”
Section: Discussionmentioning
confidence: 99%
“…Interestingly, associations of genetically predicted WMH with NDI markers at age 20 were observed primarily in white matter regions most commonly affected by WMH in older age [90,91], such as the anterior, posterior and superior corona radiata, posterior thalamic radiation, and superior longitudinal fasciculus. This corroborates recent observations that areas where WMH are most likely to appear in older adults are also those with the lowest white matter microstructure integrity on DTI in young adults [91]. In contrast, we found no association of genetically determined blood pressure, the main known risk factor for WMH, with NDI, suggesting that the association between genetically predicted WMH and NDI was likely not mediated by blood pressure.…”
Section: Discussionmentioning
confidence: 99%